The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a significant stellar population or potentially an active galactic nucleus. The radial light profile appears to diminish gradually from the core, with no distinct spiral arm features readily apparent. There's a slight elongation in its overall shape, leaning away from a perfect sphere. Faint disk-like structures appear to be present, but are not clear.

The color distribution is somewhat homogeneous across the galaxy, displaying a yellowish-white hue which suggests an older stellar population compared to actively star-forming galaxies. There is a lack of strong blue color concentrations typically associated with young, hot stars. The outer regions of the galaxy show subtle variations in color, with slight reddish tinges, indicative of a relatively small amount of dust or aging stellar populations at greater distances from the nucleus.

Based on the observed morphology and color profile, this galaxy appears to be a moderately massive system, possibly a quiescent or slowly evolving galaxy at intermediate redshift. Minor disturbances can be observed in the galaxy, potentially suggesting interactions with other galaxies.
