The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that appears yellowish, suggesting an older stellar population. The galaxy exhibits a gradual decrease in luminosity from the core outwards. There are no apparent spiral arms or significant dust lanes visible. It appears to be a quite isolated system, with no clear signs of tidal interactions or ongoing mergers, although a very slight asymmetry may hint at a past minor disturbance. The galaxy is fairly round. The overall color profile suggests that star formation activity is currently low within the galaxy.
