The galaxy appears to be a single, centrally concentrated object with a relatively smooth morphology. It exhibits a noticeable color gradient, transitioning from a bluer, possibly star-forming region in the center to a redder, more quiescent halo. The central region shows a distinct greenish hue, perhaps indicative of ionized gas emission. The overall shape is somewhat rounded, without any obvious signs of spiral arms or a bar. Faint asymmetries may be present, hinting at minor disturbances or past interactions, though a dominant merging event is not apparent.
