The galaxy presents as a relatively compact object, approximately spheroidal in shape with a slight elongation that could suggest a very weak bar or mild tidal interaction. The galaxy's central region exhibits a concentrated luminosity profile, indicative of a prominent bulge or nucleus. This central region is yellowish, suggesting an older stellar population. Fainter, diffuse bluer light surrounds the central area, which may be an indicator of ongoing, though perhaps weak, star formation in a disk or extended halo component. This is consistent with a galaxy that is past its peak star-forming epoch. There appears to be little dust. The galaxy seems to be relatively undisturbed, showing no obvious signs of a major merger event. A very faint, possible companion object is located nearby.
