This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The galaxy appears largely spheroidal in shape, being relatively round with minimal elongation. There is no clear evidence of spiral arm structures or a prominent disk. The central region displays a bright, yellowish-white hue, suggesting a population of older stars and potentially a significant bulge component. The galaxy's overall color shifts towards a redder tone, possibly indicating a dearth of ongoing star formation and a dominance of an older stellar population. The lack of significant visual disturbances, such as tidal tails or asymmetric features, suggests the galaxy has not undergone a recent major merger event. There is a slight suggestion of minor substructure in the outer regions, but the dominant impression is one of relative uniformity.
