The galaxy presents as a single, relatively smooth object. Its overall shape appears circular and regular. The light distribution is concentrated toward the center, suggesting a bulge. No distinct spiral arms or bar structures are discernible. There is a slight color gradient, with a whiter hue toward the center, possibly indicating an older stellar population, and a subtle shift toward redder colors in the outer regions. The galaxy appears largely undisturbed with no strong indications of recent major mergers or tidal interactions. There may be some minor asymmetry in the outer isophotes, suggesting some possible disturbance.
