The galaxy appears as a centrally concentrated object with a smooth morphology. Its shape is generally elliptical, exhibiting a moderate elongation. The core region presents a bright, condensed area which gradually fades outward, forming a diffuse halo surrounding the central bulge. The galaxy displays a color gradient, with the core appearing more bluish-white, indicative of a population of younger stars. The outer regions exhibit a slightly redder hue, suggestive of a greater proportion of older, cooler stars. There is no clear evidence of spiral arms or a prominent disk structure. The overall appearance is consistent with an early-type galaxy, possibly an elliptical or lenticular system, showing little to no ongoing star formation. There are some minor disturbances present.
