The galaxy presents a generally smooth, elliptical morphology. There appears to be a concentrated central bulge with a diffuse, extended halo. The color of the bulge is yellowish-orange, suggesting an older stellar population. The outer regions of the galaxy display a slightly bluer hue, possibly indicating the presence of younger stars, although the overall star formation rate appears relatively low. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy appears largely undisturbed, with no indications of ongoing major mergers or tidal interactions. It is generally round in appearance, with only a slight deviation from perfect circularity. Based on the apparent colors and lack of distinct features, it's likely a massive galaxy dominated by older stars.
