The galaxy presents as a slightly elongated, elliptical object. The light distribution appears smooth and centrally concentrated, with a bright, yellowish core that gradually diffuses outwards. Fainter, bluer light surrounds the core, extending along the major axis of the ellipse. No distinct spiral arms or bar structures are discernible within the observed optical wavelengths. The outer edges of the galaxy fade smoothly into the background sky, indicating a gradual decline in stellar density. There are no apparent signs of major tidal disturbances or ongoing mergers. The morphology suggests a relatively evolved system, likely dominated by older stellar populations in the central region.
