The galaxy presents a distinct spiral morphology, with visible spiral arms emanating from a bright central bulge. The arms appear somewhat flocculent, suggesting active star formation regions distributed along their length. There is a noticeable disk component. The color of the galaxy shifts from a yellowish hue in the central bulge to a bluer tint within the spiral arms, indicative of differing stellar populations. The arms do not appear symmetric, and there may be some disturbance. The overall shape of the galaxy is elliptical, with the spiral arms wound tightly. There may be a bar structure across the galaxy, but it is not clear. The central bulge is prominent, suggesting a galaxy with a significant spheroidal component.
