The galaxy exhibits a disk-like morphology, although it is not perfectly edge-on. Faint spiral arm structures are discernible within the disk. A bar feature is potentially present, but not pronounced. The central bulge appears moderate in size, contributing substantially to the galaxy's overall luminosity. The light from the galaxy is of a range of color suggesting varying stellar populations. The disk shows a bluer hue in the spiral arms, and the bulge is somewhat yellow. There are no readily apparent signs of a major merger event, although a possible minor disturbance cannot be ruled out. The galaxy is relatively smooth in appearance, with some signs of disk features.
