This galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light distribution suggests an older stellar population, potentially with a lower star formation rate. It appears somewhat elongated, without any clear spiral arm structures or strong indications of recent major mergers. Faint, diffuse light surrounds the central region, possibly indicating a halo of older stars or intracluster light. There is a slight asymmetry in the outer isophotes, suggesting possible minor interactions or disturbances, but the overall morphology is largely undisturbed. Color gradients suggest a central concentration of older, redder stars and a possible slight bluing in the outer regions.
