The galaxy presents as a smooth, elliptical-like object with a concentrated central bulge. The light distribution appears fairly uniform, lacking distinct spiral arm structures or prominent dust lanes. It exhibits a yellow-orange hue, suggesting a population of older stars. The galaxy appears relatively isolated, without any obvious signs of major tidal disturbances or ongoing mergers. The shape is nearly circular, showing only a slight deviation from perfect roundness. The size suggests a moderate scale, not appearing excessively large or small compared to other galaxies in the observed field. No distinct features indicative of active star formation are discernible based on color. Overall, the galaxy is likely a massive, quiescent system with a low star formation rate.
