The galaxy appears to be a disk galaxy with a noticeable bulge, but it is not perfectly circular, hinting towards possible interactions. There is evidence of some form of disturbance within the galaxy; the disk structure is not entirely smooth, and there might be subtle tidal features present. The central bulge exhibits a yellowish-orange hue, likely indicating an older stellar population. The disk shows a mixture of colors, with some bluer regions suggestive of ongoing star formation and some yellower regions that contain older stars. The galaxy is relatively compact.
