The galaxy presents a relatively smooth and round appearance, suggesting an elliptical morphology. There is no strong evidence of a prominent disk structure. A faint, blue arm or tidal feature appears to extend from the right side of the galaxy, hinting at a possible past interaction. The galaxy exhibits an older stellar population, as evidenced by its yellow-red hue, indicating that star formation may be suppressed. There are no visible signs of active star formation regions. There appears to be a secondary central core, likely a feature of a recent merger. The mass is large, and the galaxy's shape, smooth features, and suppressed star formation are all consistent with an evolved system.
