The galaxy exhibits a distinct spiral structure, displaying prominent arms emanating from a central bulge. The winding of these arms appears moderately tight. Two arms are particularly noticeable. A significant portion of the galaxy's light emanates from the central bulge, though a disk is apparent. There is no obvious bar structure present. Evident color variations exist, with a slightly yellower core transitioning to bluer hues in the outer arms, potentially indicating different stellar populations. The overall morphology suggests that the galaxy is not currently undergoing a major merging event, though there may be evidence of some disturbances, giving it an irregular shape.
