The galaxy presents a predominantly smooth morphology. There is minimal visible structure, such as spiral arms or a prominent bar. The galaxy appears roughly elliptical in shape, exhibiting a high degree of circularity. There is no evidence of significant tidal disturbances or ongoing major mergers. There may be a small, subtle asymmetry in the light distribution, but it is not definitive. The galaxy's color is primarily in the blue range, suggesting a population of young, hot stars. The light is concentrated, suggesting a fairly evolved system with ongoing star formation.
