This galaxy presents as a relatively compact, elliptical-like structure. Its light is concentrated towards a bright, yellowish core, suggesting a significant population of older stars. There appears to be a smooth decline in luminosity outward from the center, with a faint, diffuse halo. Little to no evidence of spiral arms or prominent dust lanes is visible. The overall morphology suggests a system that is either an elliptical galaxy, or a lenticular galaxy with a dominant spheroid component. There is no evidence of recent or ongoing major mergers or tidal disturbances. The round shape indicates there has likely not been a recent major merger. The galaxy shows signs of low star formation.
