The galaxy presents as a relatively bright, elliptical structure. It exhibits a smooth, centralized concentration of light, suggesting a dominant bulge component. There's a gradual decrease in luminosity from the core outwards, transitioning into a more diffuse halo. The color appears to be generally reddish-yellow, indicative of an older stellar population with less ongoing star formation, although the bluer hue in the outer reaches of the halo might signify some minor star forming regions. There are no distinct spiral arms, bars, or other prominent features typically associated with disk galaxies, and shows little visual evidence of significant recent merger activity. The estimated physical size indicates it is a massive system.
