The galaxy presents as a spiral type, exhibiting a prominent central bulge surrounded by a well-defined disk. The disk structure is characterized by spiral arms that appear somewhat tightly wound closer to the bulge but become more diffuse at the outer edges of the galaxy. These spiral arms display a mottled appearance, suggesting regions of active star formation or dust obscuration.

The bulge region is luminous and appears relatively smooth and featureless. There are areas of blue color across the disk which are indicative of younger stars. 

The overall form is elliptical. The appearance indicates that the galaxy is not undergoing a major merger, though minor disturbances may be present.
