The galaxy presents as a spiral type, seen at an oblique angle, but not quite edge-on. The disk is readily apparent with evidence of spiral arm structure, though the arms are not tightly wound. There appear to be two prominent arms emanating from the central bulge region.

A bar structure is suspected through the center of the galaxy, appearing moderately pronounced. A distinct central bulge dominates, though a considerable amount of disk is visible. Dust lanes are subtly visible along the spiral arms.

The color index indicates a relatively active star-forming region, with bluer hues apparent within the spiral arms and disk, while the central bulge appears yellower. Overall, there is no evidence of a major ongoing merger or tidal disturbance.
