The galaxy presents as a spiral type, seen at an angle slightly off from face-on. The central bulge is prominent, exhibiting a concentrated and bright yellowish-white hue. Surrounding the bulge, the disk displays some discernible spiral arm structure, with a patchy distribution of bluer regions indicative of star formation activity. The spiral arms do not appear tightly wound. There is no prominent bar structure visible through the disk. The overall impression is of a relatively undisturbed galaxy, with no obvious signs of major mergers or tidal disruptions.
