The galaxy presents as a concentrated, luminous elliptical. Its overall form appears smooth and largely featureless, lacking distinct spiral arms or prominent dust lanes. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars in this region. The luminosity gradually decreases toward the outer edges of the galaxy, forming a diffuse halo. The galaxy has a slight ellipticity. There is no evidence of significant tidal disturbances or merging activity in this image. The color index indicates a population of older stars. Star formation appears low.