The galaxy presents as a slightly elliptical, diffuse object with a smooth texture. Its color gradient shifts from a central yellowish-orange hue to a bluer, greenish tint at its outer edges. The overall structure suggests a relatively evolved system, with no obvious signs of spiral arms or a prominent disk. There are no strong indications of significant ongoing star formation, and the light profile suggests that the bulk of the stellar population resides within the central region, and the outskirts are more quiescent. The galaxy shows a slight elongation, which suggests a possible prolate spheroid. The smoothness may indicate that any past mergers have largely settled into its current morphology.
