The galaxy exhibits an elliptical morphology, appearing as a generally smooth and somewhat elongated structure. The central region displays a bright, concentrated luminosity, suggesting a higher density of stars and potentially an active galactic nucleus, though further spectral analysis would be required to confirm this. The color gradient transitions from a yellowish-white core to a bluer hue in the outer regions. This may indicate the presence of younger stellar populations in the galaxy's outer parts. The object is generally undisturbed, showing no obvious signs of major mergers or tidal interactions. However, there are hints of slight asymmetry along its major axis. The galaxy appears to have a substantial mass, given its size and overall luminosity. Star formation appears present but not dominant.
