The galaxy presents as a roughly elliptical or lenticular system, appearing largely smooth with a concentrated central bulge. The light profile suggests a relatively old stellar population, dominated by redder wavelengths, especially in the central region. There's a subtle disk-like component, although it is not sharply defined. Some areas exhibit a bluer color, which indicates the presence of younger star formations. The overall structure appears relatively undisturbed, with no obvious signs of a major merger event. There might be evidence of minor disturbances, given the asymmetry in color distribution, potentially the result of minor interaction with another galaxy. The galaxy's apparent angular size is small, indicating a substantial distance.
