The galaxy presents as a relatively well-defined disk galaxy. The central bulge is prominent and appears to be largely spheroidal in shape, with a concentrated luminosity. The spiral arms are somewhat diffuse, and loosely wound. The overall color of the galaxy suggests an older stellar population, with a more pronounced red component within the central bulge. Some blue regions are visible in the disk, indicating more recent star formation. There is no major visual disruption to the galaxy's structure suggesting this is not currently undergoing a major merger. There is a hint of a bar structure present. The galaxy has an estimated size of approximately 6.7 kpc.
