The galaxy presents as a somewhat smooth, elliptical-like structure. Its core exhibits a concentrated, yellowish-white hue, indicating a population of older stars. A faint, greenish halo surrounds the central region, possibly indicative of low-level star formation or ionized gas. The outer regions of the galaxy fade into the background with no distinct spiral arm structure or significant dust lanes visible. Overall, the morphology suggests a relatively evolved system with minimal ongoing major star formation activity. Some slight disturbances appear in the edge, indicating it may be undergoing a minor merger.
