The galaxy presents a largely smooth morphology. The central region exhibits a concentrated, bright core, indicative of a significant stellar population. The light is yellowish-red, suggesting a population of older stars. The isophotes appear generally round. There is very faint evidence of a possible extended halo or tidal feature emanating from the upper region of the core, though its nature cannot be determined with certainty from this image alone. This faint extension could be a result of past interaction or internal activity. Overall, the galaxy appears relatively undisturbed with no obvious spiral arms or disk-like structure visible.
