The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. There is a lack of discernible spiral arm structure or a prominent galactic disk. The light profile suggests a concentration of luminosity towards the center, fading gradually towards the edges. Color analysis reveals a central region that is more yellow/gold, possibly indicative of an older stellar population. The outer regions exhibit a slightly bluer hue, although not intensely so, suggesting some ongoing, but possibly subdued, star formation activity. There is no obvious evidence of tidal disturbances or ongoing major mergers, though a minor disturbance cannot be entirely ruled out. The overall appearance suggests a relatively evolved system, possibly in the process of quenching star formation.
