The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, indicative of a dense stellar population or active galactic nucleus. There is some suggestion of a slight extension or potential tidal feature on one side, possibly suggesting a minor interaction or past merger event. The overall color appears relatively red, implying a population of older, cooler stars and a comparatively low rate of on-going star formation. Given the apparent lack of significant dust lanes or spiral arm structure, the galaxy appears to be a relatively evolved system.
