The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge, which gradually fades into a diffuse halo. The color profile suggests a population of older stars, indicated by the reddish-yellow hue. There's no strong evidence of active star formation regions or distinct spiral arms. The overall shape is generally rounded, though with a slight elongation, but no tidal tails or other signs of major disturbances from recent mergers are immediately apparent. Subtle irregularities in the outer halo cannot be ruled out at this resolution.
