The galaxy presents as a largely smooth, elliptical-like structure with a concentrated, bright central region, suggestive of a significant bulge component. There is little evidence of defined spiral arms or distinct features within the galaxy's disk, if one exists. The color profile indicates a generally older stellar population, with a reddish-yellow hue dominating the central regions and a slight bluer tinge in the outer regions, indicating some recent, limited star formation. The overall morphology suggests an evolved galaxy likely transitioning away from active star formation. There is no apparent major merging activity or strong tidal disturbances affecting the galaxy's structure, though it's possible a minor disturbance could be ongoing. The galaxy appears relatively isolated.
