The galaxy presents a disk-like structure observed at an oblique angle, being neither face-on nor edge-on. A central bulge is visible, appearing of moderate size and luminosity, though not dominant. Faint spiral arm structures are present but not highly defined. There is evidence of a weak bar structure within the central region. Overall, the galaxy is likely undergoing some form of interaction or disturbance. Its morphological classification would lean towards a spiral galaxy with possible signs of recent or ongoing merging activity. The galaxy appears relatively smooth, but with some subtle internal features, particularly the spiral arms. The color gradient suggests ongoing star formation, but at a relatively moderate rate.
