The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color appears to be reddish-yellow, suggesting an older stellar population, and therefore lower star formation activity. There may be a very subtle disk feature. The ellipticity is not extreme, appearing close to circular. There is some evidence of minor disturbance within the galaxy's structure, hinting at past interactions or internal dynamic processes. The galaxy appears relatively isolated.
