The galaxy presents as a concentrated, elliptical morphology, exhibiting a smooth light profile without discernible spiral arms or a prominent disk structure. The central region displays a bright, relatively uniform luminosity, suggesting a high concentration of stars. There is a slight elongation, but it is generally rounded in shape. Color gradients are subtle, but the central region appears to be slightly more yellow, potentially indicating an older stellar population compared to the outer regions, which show a hint of bluer light. There is no evidence of significant dust lanes, tidal features, or ongoing major mergers. The galaxy appears to be relatively undisturbed.
