The galaxy presents a largely smooth, elliptical morphology. The light distribution is centrally concentrated, with a gradual decrease in luminosity outwards. The galaxy appears to be moderately rounded, showing a slight elongation but not a cigar-like shape. There is a clear color gradient, with a yellowish-white core transitioning to a redder halo. No distinct spiral arms or significant dust lanes are discernible, nor are there any signs of major mergers or tidal disturbances affecting the galaxy's structure. The smooth appearance suggests a relatively evolved system, likely dominated by an older stellar population. The colors indicate ongoing star formation activity that is likely low, but redder colors indicate dust absorption.
