The galaxy appears as a centrally concentrated, luminous object with an elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the light gradually fades into a slightly bluer halo. The overall structure is relatively smooth with some indistinct or unresolved spiral arms visible, though these features are not sharply defined. There is no obvious evidence of a major ongoing merger, but some minor disturbances may be present in the outer regions. The roundness of the ellipse is fairly moderate, not strongly circular but also not highly elongated or cigar-shaped. There is no significant indication of prominent dust lanes obscuring the light from the galaxy's core or disk.
