The galaxy presents as a largely smooth, elliptical-like structure. It displays a concentrated, bright central region, suggesting a significant bulge component. The overall color is yellowish-orange, indicating a population of older stars. The galaxy appears relatively isolated, with no obvious signs of major interaction or merging events, although some minor disturbance cannot be entirely ruled out. There is a subtle elongation observed; however, the object is predominantly round in shape. There is no readily apparent disk structure.
