The galaxy presents as a well-defined elliptical morphology. It exhibits a smooth, centrally concentrated light profile with a noticeable ellipticity, appearing cigar-shaped. There's a color gradient visible; the central region displays a yellowish-red hue, suggesting a population of older stars. Fainter blue-green tones are observed in the outer regions, possibly indicating pockets of younger stellar populations. There is no obvious evidence of a spiral structure, significant dust lanes, or ongoing major merging activity. Some minor disturbances may exist at the edges. Overall, the galaxy's structure appears relatively undisturbed and evolved.
