The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The color profile is dominated by yellowish hues in the core, suggesting an older stellar population. The outer regions exhibit a faint, diffuse halo with a subtle greenish tint, possibly indicating ongoing or recent star formation activity, albeit at a lower rate than more actively star-forming galaxies. There appears to be a small area of increased red color, indicating a potential pocket of dust or an isolated region of older stars. The galaxy displays a high degree of circularity with only minor irregularities, showing no significant signs of major mergers or strong tidal disturbances. 
