The galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure. The spiral arms are readily visible, displaying a tightly wound morphology. There appears to be a moderate bar structure. There is a noticeable bulge, but it appears to be relatively small in comparison to the disk. The light distribution suggests a central concentration with diminishing brightness towards the outer regions. The color profile shows a yellowish core, possibly indicating an older stellar population, while the spiral arms exhibit a bluer hue, consistent with ongoing star formation. There appears to be a significant tidal tail coming out of the galaxy, suggesting it could have undergone a recent merger.
