The galaxy presents as a somewhat smooth, elliptical structure with a concentrated, bright central bulge. The color is primarily a yellow-orange hue in the central region, suggesting an older stellar population. There is a subtle color gradient, with the outer regions appearing slightly bluer than the core, hinting at the presence of younger stars or low-level star formation activity, however, the overall stellar formation rate is likely quite low. The galaxy appears relatively undisturbed, showing no major signs of ongoing mergers or tidal interactions, although there is a faint disklike structure to one side. It is moderately massive.
