The galaxy appears to be a spiral galaxy, though the spiral arms are not well-defined. The galaxy's central bulge is prominent and appears relatively bright. The overall color of the bulge is reddish. Surrounding the bulge is a disk component that exhibits a bluer hue, indicating the presence of younger, hotter stars. There appears to be some dust obscuration in the disk, contributing to the patchy appearance of the spiral structure. The disk is not particularly extended, and the galaxy appears relatively compact. There is some evidence of tidal disturbances or interactions with a nearby galaxy, suggesting a possible minor merger event. The overall morphology suggests that the galaxy may be undergoing some form of active galactic nucleus (AGN) activity.
