The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is little evidence of spiral arms or significant disk-like features. The color appears to be generally redder, indicating an older stellar population and possibly a lower rate of active star formation within the galaxy. The lack of distinct blue regions suggests a reduced presence of young, hot stars. It appears to be a fairly isolated galaxy, with no obvious signs of tidal disturbances or interactions with neighboring galaxies. The galaxy is more oblong than circular, and the bulge extends into the edges of the galaxy.
