The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. Its overall shape appears relatively round but not perfectly circular. The color profile is dominated by yellow and red hues, suggesting an older stellar population with a lower rate of ongoing star formation. There is very little evidence of spiral arms, disk structures, or prominent dust lanes. The galaxy exhibits a fairly compact core with a gradually decreasing luminosity towards its outer edges. There are no visible signs of any major ongoing mergers, tidal tails, or significant disturbances in its overall structure, indicating the galaxy is largely undisturbed. There are no noticeable bright blue regions, typically indicative of recent star formation. Overall, the galaxy presents as a relatively quiescent, evolved system.
