The galaxy presents a largely smooth, elliptical morphology. It appears to be relatively round, exhibiting minimal disk-like features or irregular structures. The light profile is centrally concentrated, with a bright, yellowish core that gradually diffuses outward. There is little evidence of significant dust lanes, spiral arms, or active star formation regions within the visible spectrum. The galaxy appears to be undisturbed, showing no obvious signs of ongoing mergers or tidal interactions.
