The galaxy exhibits an elliptical morphology, presenting a smooth, centrally concentrated luminosity profile with a low degree of visible substructure or spiral arm features. The shape is elongated, not perfectly circular. The galaxy displays a color gradient, with the central region appearing redder than the outer regions, suggesting a population of older stars in the core and relatively younger stars in the outer regions. The galaxy shows no strong evidence of active star formation. There is a faint stellar halo extending outwards. There is no sign of significant dust lanes or tidal disturbances, suggesting the galaxy is relatively undisturbed.
