The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The core exhibits a yellow-white hue, suggestive of an older stellar population. Proceeding outward from the center, there is a faint, diffuse halo of light. The shape is moderately elongated, appearing somewhere between round and cigar-shaped. No spiral arms or distinct dust lanes are discernible. There is no visually apparent evidence of recent or ongoing major merger activity; it is an isolated galaxy.
