The galaxy presents as a somewhat elongated, lenticular-like structure. A concentrated, bright central bulge is visible, surrounded by a fainter, more diffuse disk. There is little evidence of defined spiral arms. The galaxy exhibits a relatively smooth overall appearance, with only subtle variations in color and brightness across its structure. The shape seems to be somewhere between round and cigar shaped. There are no indications of ongoing major merger activity, although some minor disturbances may be present based on the morphology. Color gradients suggest a population of older stars.
