The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical galaxy, exhibiting a nearly spherical shape. There is a discernible core region, indicated by a higher concentration of light, which diffuses outward into a fainter halo. The color appears to be a somewhat uniform yellow-white across the galaxy, suggesting a population of older stars, with no apparent spiral arms or significant dust lanes visible in this image. There is no obvious indication of active star formation, and there does not appear to be any significant signs of a recent merger. The galaxy exhibits a fairly symmetrical profile, with a slight elongation, potentially indicating a transition between elliptical subtypes.
