The observed galaxy exhibits a disturbed morphology, suggestive of a possible interaction or merger event. The galaxy appears elongated, with an axial ratio of approximately 0.6. The central region of the galaxy is dominated by a bright bulge, with a diffuse halo extending outwards. Faint spiral arm structures are visible in the bluer wavelengths, but their organization is unclear. The overall color gradient indicates a possible active star-forming region, with the bluer regions correlating to where the spiral arms appear to be. There may be evidence of tidal tails or other morphological distortions. Dust lanes appear to be present within the galaxy.
