The galaxy presents as a centrally concentrated object with a largely smooth, featureless morphology. The light distribution suggests a spheroidal shape, though it is somewhat irregular. There is a distinct central bulge region that appears brighter and possibly slightly redder in color than the surrounding halo. Faint extensions or tidal features are not readily apparent, suggesting it is a relatively isolated system or that any past interactions are not currently evident in its overall structure. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo component. Overall, the galaxy exhibits colors consistent with a population of older stars, but there appears to be a bluer element that is more visible toward the outskirts of the galaxy.