The galaxy presents as a well-defined elliptical morphology. The core exhibits a bright, concentrated luminosity, indicative of a substantial stellar population and potential central mass concentration. The galaxy appears reddish in color, which is suggestive of an older stellar population dominated by red giant stars and a reduced rate of ongoing star formation. The galaxy's overall smooth texture further implies a lack of significant dust lanes or spiral arm structures. Its shape is elongated, with a cigar-shaped appearance, which potentially indicates that it is in the process of merging. There is some evidence of possible tidal features, likely a result of an old merger or disturbance.
