The galaxy appears as a centrally concentrated object with a slightly diffuse halo. It presents a generally elliptical morphology, though not perfectly spherical; the shape tends toward an in-between rounded form. There is no strong evidence of a prominent disk structure or spiral arms visible in this image. The central region exhibits a bright concentration of light, suggesting a substantial stellar population. Faint, extended features may be present, indicating possible tidal disturbances or interactions, although no clear signs of a major merger are evident. The color profile suggests a relatively evolved stellar population.
