The galaxy presents as a generally smooth and elliptical structure. It exhibits a concentrated central bulge that is bright, with a yellowish hue, suggesting a population of older stars. A fainter, somewhat elongated halo surrounds the core. There are subtle hints of asymmetry or tidal features surrounding the main body of the galaxy, possibly indicating a minor gravitational interaction or recent merger event, or perhaps faint spiral arms that are difficult to resolve. The colors appear to be consistent with an older stellar population. The outskirts of the galaxy are relatively diffuse, lacking distinct features. The galaxy appears to be in an intermediate stage of evolution, having largely exhausted its gas supply for star formation, though some small amount may still be present.
