The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. A faint, extended halo or disk is present around the central region. There appears to be a subtle color gradient, with a slightly bluer hue visible in the outer regions of the disk compared to the more yellow/red-shifted central bulge. This suggests the possibility of ongoing, although low levels, star formation in the outer regions while the bulge is populated with an older stellar population. No significant tidal disturbances or merging features are obvious in the immediate vicinity of the galaxy.
