The galaxy presents as a centrally concentrated, luminous system with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The overall light distribution falls off gradually from the center, lacking any prominent spiral arm structures or distinct features. There is a slight elongation to the galaxy's shape, appearing more "in-between" round and cigar shaped. Minor disturbances might be present, but overall the galaxy appears to be isolated. The observed color gradient, from yellowish-white in the core to slightly redder hues in the outer regions, indicates a potential radial variation in stellar populations, possibly with older, redder stars dominating the outer regions.
