The galaxy presents a disk-like morphology, with a prominent central bulge. The bulge appears moderately sized, contributing significantly to the overall luminosity. The galaxy exhibits a bar structure extending across a substantial portion of the disk. There appear to be spiral arm features, but they are not well-defined. The overall colour suggests a composition of both older stellar populations in the bulge and younger stars in the disk, resulting in a yellow-white hue. There are no obvious signs of recent major merging activity, though there is the possibility of minor disturbances or interactions, but without more detailed data, it is difficult to say. The galaxy is viewed at an oblique angle, somewhere between face-on and edge-on.
