The galaxy appears to be a spiral galaxy with a prominent disk structure. The galaxy is tilted relative to our line of sight, presenting an oblate appearance. Spiral arms are readily discernible, appearing tightly wound around the central region. The central bulge is relatively small and exhibits a yellowish hue, potentially indicative of an older stellar population. The spiral arms are characterized by a bluer color, suggesting ongoing star formation activity within them. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions. The galaxy has a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions.
