The galaxy presents a largely elliptical morphology, appearing smooth and centrally concentrated. Its overall color is generally reddish-yellow, suggesting a population of older stars and a relatively low rate of on-going star formation. There is no visible dust lane or spiral arm structure. The galaxy displays a slight color gradient, with the central region appearing more intensely yellow and the outer regions exhibiting a subtle blueish halo. The halo suggests the presence of a sparse population of younger stars extending beyond the main body of the galaxy. No obvious signs of tidal tails or morphological disturbances are apparent, and it seems to exist in relative isolation.
