The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge. Its color gradient suggests a relatively older stellar population, with a yellowish hue dominant throughout the galactic structure. No distinct spiral arms or significant dust lanes are visible. The overall appearance indicates a system dominated by stars with subdued star formation activity. The shape of the galaxy appears to be somewhere between round and elliptical, with no cigar-like elongation. There is no visible evidence of on-going major or minor merging events, only small disturbances.
