The galaxy presents a roughly elliptical morphology, appearing somewhat elongated rather than perfectly spherical. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. Light distribution decreases gradually outwards from the center towards the edges. Color variation is observed, with a yellowish hue dominating the core, likely indicative of an older stellar population. The outer regions show bluer tones suggesting the presence of younger stars. Some asymmetry can be seen in the image, but it is difficult to determine whether it is due to internal structure or external interactions without higher resolution imaging. Overall the galaxy appears to be relatively smooth with little to no distinct spiral arm structure. Star formation appears to be present, but overall low. The estimated redshift of the object indicates that it is a relatively distant galaxy.
