This galaxy appears to be a spiral galaxy, viewed at a relatively high inclination angle. There is evidence of a disk structure. The galaxy exhibits a central bulge, but it does not appear to be the dominant feature. Spiral arms are visible extending from the central bulge into the disk. Faint evidence of a bar structure exists, but not very prominent. Overall, the galaxy does not appear to be undergoing any major merging events or significant disturbances. The color gradient suggests ongoing star formation within the disk.
