The galaxy presents as a concentrated, elliptical-like structure with a high degree of central luminosity. The core region exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. A faint, diffuse halo surrounds the core, extending outwards with a gradual decrease in surface brightness. There are slight hints of non-uniformity in the halo's texture, but no clear spiral arm structures or distinct features are immediately apparent. The color profile indicates a higher concentration of older, redder stars, which are characteristic of evolved galaxies with suppressed star formation rates. Overall, the galaxy appears relatively smooth, with a possible minor disturbance visible.
