This galaxy exhibits a disk-like morphology, viewed at an oblique angle to our line of sight. A central bulge is readily apparent, appearing yellowish-white and smoothly textured, suggestive of an older stellar population. Surrounding the bulge is a flattened disk component. The disk displays a more mottled texture with hints of spiral arm structure, although these are not sharply defined. The disk's color is bluer than the bulge, indicating the presence of younger, hotter stars and ongoing star formation. Dust lanes may be present, contributing to the mottled appearance of the disk, though resolution limitations prevent clear delineation. The galaxy appears moderately elongated, with a major axis that is approximately twice the length of its minor axis. There is no obvious evidence of a recent major merger, though subtle tidal features cannot be ruled out. The outer edges of the galaxy fade gradually into the background sky.
