The galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is evidence of spiral arm structure, although the arms are somewhat tightly wound. The central bulge appears moderately sized, exhibiting a yellow-red color indicating an older stellar population. The arms show a bluer hue, indicative of younger stars and potentially ongoing star formation. There is also a likely central bar structure. The morphology suggests a galaxy that has experienced some level of interaction or disturbance.
