The galaxy presents as an elliptical form, appearing largely smooth and relatively featureless. Its color profile indicates a higher concentration of older stellar populations, trending towards redder wavelengths. The object exhibits a moderate degree of roundness, deviating from a perfectly spherical shape. There is no visible evidence of ongoing major mergers or significant tidal disturbances. Based on the overall morphology, this galaxy is likely a mature system with a low specific star formation rate. Its half-light radius suggests a compact nature, considering its estimated distance.
