The galaxy presents as a single, relatively smooth object with a slightly elliptical shape. There is a central, bright bulge that appears generally round, showing a concentration of older stars. Fainter extended light surrounds the central bulge, possibly representing a diffuse stellar halo or a faint disk component. There is some evidence of recent or ongoing star formation, as indicated by the faint bluish-green hue within the galaxy's outskirts, though star formation rates appear to be relatively low overall. There might be very minor disturbances in its form, though the galaxy generally appears isolated. No obvious tidal tails or interacting companions are visible within the immediate vicinity, suggesting it has likely evolved in relative isolation.
