The galaxy presents as a single, relatively symmetrical object. It displays a smooth, somewhat elliptical morphology, with a noticeable concentration of light towards the center, suggesting the presence of a central bulge. There is minimal evidence of distinct spiral arms or a prominent disk structure. The galaxy exhibits a yellowish-orange hue. No obvious signs of ongoing major mergers or tidal disturbances are apparent. The overall appearance indicates a relatively evolved system, likely with a significant population of older stars.
