The galaxy presents as a disk galaxy, seen at an oblique angle. It exhibits a smooth, centrally concentrated morphology. The central region appears yellowish, potentially indicating an older stellar population or dust obscuration. Progressing outwards from the center, the disk shows hints of spiral structure, marked by subtle color variations. Faint blue tinges are visible in these spiral regions, possibly indicating pockets of younger, hotter stars associated with ongoing star formation. The galaxy does not appear to be undergoing any major mergers or interactions. There is no clear evidence of a bar structure. The overall appearance suggests a relatively evolved galaxy, potentially somewhere on the transition between a spiral and a lenticular galaxy.
