The galaxy presents an elliptical morphology, appearing generally smooth in structure with no discernible spiral arms or distinct disk component. The light distribution seems relatively uniform across the galaxy's body, suggesting an older stellar population. There is a slight color gradient visible, with the core appearing somewhat more yellow/red and the outer regions tending towards bluer hues, potentially indicating subtle variations in stellar ages or metallicities across the galaxy. Overall, the galaxy seems to be an early-type system without significant recent star formation. There is some indication of possible tidal disturbances and potentially merging characteristics. The galaxy exhibits a moderately luminous core.
