The galaxy presents as a largely smooth, elliptical-like structure, with a concentrated central bulge that gradually fades into the outer regions. The color profile suggests an older stellar population, with a dominant yellow-orange hue in the core, hinting at the presence of evolved stars. Fainter, bluer colors are present in the more diffuse outer regions, suggestive of recent star formation. The galaxy appears undisturbed, showing no signs of major mergers or tidal disruptions. Overall, the galaxy appears to be relatively massive with low star formation.
