The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears to be the brightest region. There's a gradual decrease in luminosity moving outward from the core, suggesting a radial profile that declines smoothly. The overall color profile is more weighted towards the redder end of the spectrum, with the central area more yellow/gold, indicating an older stellar population. There are no obvious dust lanes or spiral arm structures visible in this image. The galaxy appears relatively isolated, with no clear signs of ongoing major mergers or significant tidal disturbances.
