The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color appears to be in the yellowish-orange range, suggesting a population of older stars, potentially indicating minimal ongoing star formation. The galaxy appears moderately luminous. Its shape is somewhat rounded, with a subtle deviation from a perfect sphere, showing a hint of ellipticity, but not leaning towards a highly elongated or cigar-like form. There is no evidence of significant tidal disturbances or ongoing mergers, although subtle asymmetries might indicate minor gravitational interactions in its past or present. Overall, the galaxy presents the characteristics of a mature, relatively undisturbed system.
