The galaxy presents as a spiral type, exhibiting a moderate central bulge. Spiral arms are visible, though tightly wound around the central bulge. The overall color of the galaxy appears to be relatively homogenous, with a subtle bluer tint to the outer edges of the spiral arms, suggesting ongoing, though perhaps subdued, star formation in those regions. There is no obvious sign of major ongoing merger activity, however, there are some minor indications of possible gravitational disturbance. The nucleus is bright and concentrated, suggestive of older stellar populations.
