The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-orange hue, potentially indicative of an older stellar population dominated by red giant stars. The light distribution appears generally spheroidal with moderate ellipticity; there is little visual evidence of spiral arms or a distinct disk structure. Faint, diffuse extensions of light emanate from the central region, contributing to a gradual decrease in luminosity with increasing radial distance. There appear to be no significant signs of tidal disturbances, such as extended tails or distorted features, suggesting it has likely not recently undergone a major merger event. The overall color suggests limited on-going star formation.
