The galaxy presents an overall elliptical morphology, with a centrally concentrated bulge exhibiting high surface brightness. It appears to be an early-type galaxy, lacking prominent spiral arm structures. The central region is bright and compact, indicating a potentially dense stellar population. The outer regions show a gradual decrease in surface brightness, transitioning into a diffuse halo. There are asymmetries and disturbances, suggesting a recent or ongoing interaction or merger event. A faint tail or tidal feature extends from one side of the galaxy, further supporting the presence of gravitational interactions. The galaxy displays a slight color gradient, with bluer colors in the outer regions suggesting ongoing star formation, although the overall color profile indicates a predominantly older stellar population.
