The galaxy presents as a relatively compact object, generally elliptical in shape with a high degree of symmetry. The light distribution appears smooth and centrally concentrated, with a minimal disk-like component observed. The color index suggests a population of older stars dominating the light, as the object appears reddish in coloration. There is no evidence of significant ongoing star formation within the galaxy, nor the presence of any tidal features or signs of major mergers. No complex structures are discernible; there are only subtle internal variations.
