The galaxy appears to be a disk galaxy, observed at an oblique angle. It displays a relatively smooth, centrally concentrated bulge, with a flattened disk extending outwards. The central region exhibits a yellowish hue, possibly indicating a population of older stars. The outer regions of the galaxy exhibit a bluish tint, which could be indicative of ongoing star formation and a population of younger, hotter stars. There is a slight suggestion of spiral arm structure, but it is poorly defined and possibly flocculent. No obvious signs of a major ongoing merger event are apparent, however, there are some possible indications of minor disturbances in the outer disk region. The galaxy appears to be relatively isolated in the field of view.
