The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light distribution indicates a primarily spheroidal morphology, with the isophotes appearing largely elliptical. There is a hint of disk-like structure extending outward from the central region, but it is not sharply defined. The overall color suggests a stellar population that is actively forming stars, but the dominant light likely comes from older populations. There is no strong evidence of a major ongoing merger or tidal disturbance; however, there may be minor internal disturbances. The galaxy does appear to be quite circular.
