The galaxy appears to be a relatively compact object with a dominant, smooth spheroid component. The central region exhibits a yellowish-white color, suggesting an older stellar population. There is faint evidence of a possible disk or arm structure extending from the central region. This structure is subtle, not well-defined, and displays a gradient in color, shifting towards a slightly redder hue in the outer portions. A redder clump of material is present on one side of the galaxy, potentially indicative of star formation or tidal debris from a past interaction. Overall, the galaxy’s morphology hints at a system undergoing some form of interaction or disturbance, although the dominant smooth component suggests an earlier phase of its evolutionary history.
