The galaxy presents as a relatively compact and somewhat irregular object. There is a faint, diffuse halo surrounding the central region of the galaxy. Within the central region, there appears to be some substructure, perhaps indicative of spiral arms or an irregular disk. The galaxy displays a noticeable color gradient, transitioning from a bluer hue in the central regions to a redder hue in the outer regions. This could indicate differing stellar populations or dust content across the galaxy. There also appears to be minor disturbances to the galaxy, but no signs of a major merger. 
