The galaxy appears to be a spiral galaxy, with an inclination that suggests we are viewing it at an oblique angle. The central bulge is relatively prominent and appears yellowish, indicative of an older stellar population. There are hints of spiral arm structures extending outward from the bulge, but the arms are not sharply defined. The bluer color in parts of the disk may suggest areas of active star formation. The overall light distribution suggests it is a fairly massive galaxy with a relatively low star formation rate. There is evidence of morphological disturbance within the galaxy, possibly due to a minor interaction or internal processes. The outer regions appear somewhat diffuse, lacking sharp boundaries. The galaxy's shape leans towards an elliptical shape, but is in between a circle and cigar.
