The galaxy presents as a primarily smooth, elliptical-like structure. Its color profile suggests a dominant population of older stars, evidenced by the orange-red hue concentrated towards the core. There is faint indication of a disk-like structure. No spiral arms are discernible. The galaxy appears to be relatively isolated, showing no major signs of tidal disruption or interaction with other galaxies, although there might be a minor disturbance. The central bulge is prominent and appears symmetrical. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy in a relatively quiescent state.
