The galaxy presents as a disk-shaped system, with a slight inclination relative to our line of sight. It exhibits a central bulge that appears luminous, suggesting a concentration of older stars. Surrounding the bulge, there is a disk component, with visible signs of spiral arm structure, though these are somewhat diffuse and flocculent. The overall color of the galaxy appears to be leaning towards a yellow-white, which is consistent with an older stellar population throughout the galaxy. There is some indication of ongoing star formation with a slight blueish tinge in parts of the disk. A possible minor tidal disturbance, such as a small plume or asymmetry in the outer disk, could be present. There does not appear to be a bar structure. The galaxy is of moderate size for a spiral system.
