The galaxy presents a primarily smooth, elliptical morphology with a moderate degree of roundness, though it appears more in between round and elongated rather than perfectly circular. There is no obvious spiral structure or distinct disk component visible in this image. Evidence of any major merger events or strong tidal disturbances is not apparent, although a minor perturbation cannot be ruled out. The galaxy exhibits a concentrated light profile with a significant central bulge. The color appears somewhat redder, indicating a population dominated by older stars, and a generally low star formation rate is expected. The galaxy has a high mass. The overall impression is of a relatively evolved galaxy.
