The galaxy appears to be a relatively smooth, elliptical system. The light is concentrated towards the center, indicative of a prominent bulge. The radial light profile decreases smoothly without distinct spiral arm features, though some faint hints of a disk structure cannot be ruled out. The overall color of the galaxy appears to be yellowish-white, suggesting a population dominated by older stars with relatively little ongoing star formation. The galaxy exhibits a fairly regular elliptical shape with a slight deviation towards a more flattened, or "in-between" shape, exhibiting only very slight asymmetries that could indicate a past or ongoing minor merger event. There are no obvious signs of strong tidal tails or other major disturbances to the galaxy's structure. The core region appears to be brighter than the surrounding areas, and the isophotes, while generally smooth, show some irregularities, which suggest recent activity or interactions.
