The galaxy presents as a smooth, elliptical-like structure, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. Its overall shape appears to be in-between round and cigar shaped. The galaxy's color profile is dominated by redder wavelengths, suggesting an older stellar population. There are some faint indications of minor disturbances in the galaxy's morphology, hinting at possible past interactions or internal dynamics. Despite these minor features, the galaxy appears largely undisturbed, with no major signs of ongoing merging activity.
