The galaxy appears as a diffuse, centrally concentrated object. The overall morphology suggests a spiral or lenticular galaxy seen at a slight angle. The central bulge region exhibits a bright, yellowish-white hue. The outer disk appears fainter and exhibits hints of blueish and reddish tones, potentially indicating regions of differing stellar populations or dust obscuration. While a spiral structure is not clearly visible, the asymmetrical distribution of the blueish component suggests the presence of faint spiral arms. There is a slight disturbance in the morphology of the disk, which may indicate a minor interaction with another galaxy or past merger event. The general smoothness of the galaxy suggests that it is mostly comprised of older stars, but the presence of cooler gases leads to some star formation.
