The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a well-defined, centrally-peaked profile with a gradual fall-off in intensity towards the edges. The galaxy exhibits a warm color, transitioning from a yellowish core to reddish outer regions. There is very little evidence of spiral arms or significant dust lanes. No obvious signs of ongoing major mergers or tidal disturbances are apparent; however, subtle asymmetry in the outer regions may indicate a past interaction or minor disturbance. Overall, the galaxy presents as a mature system dominated by an older stellar population, possibly with a small amount of recent star formation activity.
