The galaxy presents a prominent spiral structure. Its arms appear somewhat tightly wound near the central bulge, transitioning to a more open structure at their periphery. The central bulge is luminous, exhibiting a smooth, concentrated light profile. The spiral arms show patchy regions of star formation activity, indicated by localized areas of bluer light. The overall color suggests a mix of stellar populations, with a noticeable gradient from the yellowish central region towards bluer outer regions within the spiral arms. The galaxy exhibits a defined disk and shows no obvious signs of major mergers, though some minor disturbances cannot be ruled out. The galaxy's morphology indicates a classic spiral structure with a moderately sized bulge. Two spiral arms are clearly visible extending from the central bulge.
