The galaxy presents a generally smooth morphology, with a highly rounded shape, exhibiting characteristics of an elliptical galaxy. The light distribution appears concentrated towards the center with decreasing luminosity as it extends outward. There is little to no indication of spiral arms or a distinct disk structure. The primary color appears to be in the redder part of the spectrum, suggesting a population of older stars. There may be a few subtle disturbances present, but generally, the system does not exhibit significant signs of ongoing or recent merger activity.
