The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated distribution of light. It exhibits a generally rounded morphology. There is a suggestion of minor disturbance on the outskirts, possibly indicative of a past or ongoing interaction or minor merger event. The galaxy's color suggests a relatively older stellar population. The overall structure appears somewhat complex, possibly a result of an ongoing or past galactic interaction. Further analysis would be required to determine the exact nature of these disturbances.
