The galaxy presents as a centrally concentrated structure, likely an elliptical or lenticular galaxy based on its overall smooth appearance. It has a somewhat elongated shape. The galaxy exhibits a gradual radial decrease in surface brightness from the core outwards. There is some subtle, mottled texture in the galaxy's halo, potentially indicating the presence of unresolved stellar populations or faint substructures. The central region appears more blueish, and the outer regions appear redder. There is no clear indication of spiral arms, a prominent dust lane, or a significant nuclear point source. There might be a minor disturbance in the structure of the galaxy, but it is not enough to classify it as an actively merging system.
