The galaxy appears to be a fairly smooth elliptical galaxy, with a dominant central bulge and a lack of readily discernible spiral arms or a distinct disk structure. The color profile suggests the presence of an older stellar population; there appears to be a lack of significant recent star formation, supported by the apparent lack of blue color. It displays an overall round morphology, with a minor axis to major axis ratio close to 1. Subtle irregularities in the isophotes may indicate minor tidal disturbances or past interactions, but overall, the galaxy appears relatively undisturbed, with no evidence of major mergers or significant ongoing star formation. The galaxy's luminosity profile appears centrally concentrated, consistent with an early-type galaxy.
