This galaxy presents as a largely homogenous, elliptical structure, exhibiting a smooth light distribution. The core region displays a concentrated luminosity, transitioning to a gradually fainter halo. Overall, the galaxy appears as a fairly symmetrical, rounded object. There is very little evidence of any significant disk-like features or spiral arms. No major morphological disturbances are apparent; the galaxy is likely relaxed. The color profile suggests a population of older stars, with a greater contribution in the redder end of the spectrum.
