The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated, bright core region, suggesting a significant accumulation of stellar mass in the central bulge. The light distribution is dominated by yellow and orange hues, indicating a population of older stars and a relatively low rate of ongoing star formation. Faint, diffuse extensions are visible around the central region, possibly a halo of older stars or the result of past mergers. There are no apparent spiral arms or distinct dust lanes visible in the image. The overall morphology suggests a relaxed system that has largely completed the process of hierarchical assembly. The slight elongation may indicate it is a classifying as an E4-5 galaxy on the Hubble scale.
