The galaxy presents a predominantly smooth, elliptical morphology. The core region exhibits a concentrated and bright appearance, suggesting a relatively high stellar density. A subtle asymmetry is noted in the galaxy's overall structure. A possible merging event, or interaction with a smaller companion, cannot be excluded based on the presence of minor structural disturbances. The galaxy displays a moderate red color, potentially indicating an older stellar population and a lower rate of ongoing star formation. There appears to be a faint, diffuse halo surrounding the main body of the galaxy, however it is difficult to discern.
