The galaxy appears to be a relatively smooth and rounded elliptical galaxy. Its light profile suggests a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The galaxy exhibits a generally uniform color, indicating an older stellar population and a lower rate of current star formation. There are no prominent spiral arms or significant dust lanes visible. It does not appear to be undergoing any major merging events. The overall structure is well-defined and shows no obvious signs of significant tidal disturbances or ongoing interactions with neighboring galaxies. The galaxy has a moderate size.
