The galaxy presents a generally smooth and elliptical morphology, exhibiting a moderate ellipticity. Its light profile appears relatively concentrated, with a gradual decrease in luminosity from the center outwards. The galaxy's color index suggests a dominant population of older stars, visible by its yellow/red hue. There are no clear signs of spiral arms or a distinct disk structure. Faint indications of minor disturbances in its symmetry are visible. There is no evidence of a recent or ongoing major merger. The overall appearance indicates a relatively evolved system with suppressed current star formation. The size implies it is of an average size.
