The galaxy presents as a relatively smooth, elliptical-like structure, though it appears somewhat elongated. Its color profile suggests an older stellar population, with a noticeable concentration of yellow and red hues towards the central bulge. There is little evidence of recent star formation. Faint, diffuse light extends outwards from the central region, indicating a gradual decrease in stellar density with increasing distance from the core. The galaxy is not perfectly spherical and has what appears to be a faint disk extending horizontally. Based on its morphology, the galaxy appears to be undisturbed, without any obvious signs of recent major mergers or tidal interactions.
