The galaxy presents as a relatively small, elliptical-like structure with a smooth, concentrated appearance. The light is fairly uniform, with no obvious dust lanes or spiral arm structures visible. The galaxy's color indices suggest a population of older stars, resulting in a redder overall hue. There appears to be a centrally concentrated region, possibly indicating a bulge or a bright galactic nucleus. The outer edges of the galaxy gradually fade into the background, suggesting a low-density stellar halo. Based on its overall morphology, this galaxy appears to be in a relatively quiescent state, with potentially low ongoing star formation.
