The galaxy presents as a centralized, largely featureless object. Its overall color profile suggests a bias toward older stellar populations. The central region is brighter and more concentrated, implying a possible bulge component. There is minimal visual evidence of a disk-like structure or spiral arms. Faint extensions are observed in the periphery, although the resolution limits detailed morphological classification. There are no signs of major ongoing merging activity; the morphology indicates a relatively undisturbed system.
