The galaxy presents as a relatively compact, elliptical morphology. Its core exhibits a bright, concentrated region that transitions smoothly outwards. The color profile suggests an aging stellar population, with a reddish-orange hue dominating the central region. This potentially indicates a lack of significant ongoing star formation in the core. Moving outward from the nucleus, a faint, diffuse halo is observed, exhibiting a slightly bluer color, which could signify the presence of younger stars in the galaxy's outer regions, or more simply represent an artifact from the imaging process. There is no distinct spiral arm structure detectable. No signs of major tidal disruption or mergers are visually apparent. Overall, this galaxy appears to be a well-formed and settled system.
