The galaxy presents as a somewhat elongated structure, appearing intermediate in shape between a round and cigar-shaped morphology. It exhibits a relatively smooth overall appearance, with a dominant central bulge characterized by a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions extend outwards from the central bulge, implying the presence of some ongoing star formation within the galaxy. There are no indications of major mergers or strong tidal disturbances, though the presence of a very slight distortion cannot be ruled out. The overall color profile indicates a generally evolved stellar population.
