This galaxy presents a relatively compact morphology. The light profile appears centrally concentrated, with a smooth, slightly elliptical overall shape. While a disk-like structure can be inferred, distinct features or spiral arms are not readily apparent. There is evidence of possible minor disturbances; a faint plume or tidal tail extending from the galaxy is observed, indicating a potential past interaction or merger. It seems the galaxy could be the later stage of a merger. Color gradients within the galaxy are evident, transitioning from a bluer central region to redder colors in the outer regions. This could suggest a younger stellar population at the center and older stellar populations farther out. 
