The galaxy presents as a disk galaxy, inclined at an angle, though not quite edge-on. A central bulge is apparent, exhibiting a yellow-white hue, indicative of an older stellar population. Fainter spiral arm structures extend outwards from the bulge. These arms appear somewhat patchy, and display a bluish tint, suggesting the presence of younger, hotter stars and ongoing star formation. The morphology is predominantly disk-like, yet the arms appear somewhat disturbed or irregular, perhaps hinting at a minor interaction. No strong tidal features are visible, suggesting any interaction is of low intensity or occurred in the distant past.
