The galaxy presents a generally elliptical morphology with a smooth, concentrated central bulge that exhibits a bright yellowish-white hue, indicating a population of older stars. The outer regions of the galaxy fade gradually into a more diffuse halo with a subtle blueish tint, suggesting some recent or ongoing star formation. The galaxy appears elongated, with a major axis significantly longer than its minor axis, exhibiting a moderate flattening. There is no clear evidence of spiral arm structures or strong dust lanes. Faint tidal features are not obviously present, implying it is not currently undergoing a major merger. Overall, this galaxy appears to be a relatively quiescent system.
