The galaxy presents as a spiral type, viewed at a significant inclination. A distinct bulge dominates the central region, exhibiting a yellow-white hue. The disk component is evident, with hints of spiral arm structure. The arms appear somewhat flocculent. The dust lanes are subtle but perceptible, contributing to the patchy appearance of the disk. There is a possibility of a bar structure within the central bulge. Overall, the galaxy appears relatively smooth, with no obvious signs of major mergers or strong tidal disturbances.
