The galaxy presents as a centrally concentrated object with a smooth overall appearance. It exhibits a slightly elongated, elliptical shape. A bright, yellowish core dominates the central region, suggesting a high concentration of older stars and potentially a supermassive black hole actively accreting material.

Moving outward from the core, the galaxy transitions to a more diffuse halo. The halo is composed of a fainter, bluish light, indicating the presence of younger stars and ongoing star formation, though to a lesser degree than the core. There are some minor, irregular disturbances in the outer regions, possibly suggestive of past interactions or mergers. The galaxy appears relatively isolated, without obvious signs of a major ongoing merger or tidal disruption.
