The galaxy presents a notable disk-like morphology, although it isn't perfectly face-on, possessing a slight inclination relative to the observer's line of sight. Within the disk, clear indications of spiral arm structures can be observed. These arms appear somewhat tightly wound close to the central bulge, gradually becoming looser toward the outer regions of the disk.

The central bulge constitutes a prominent feature of the galaxy, exhibiting a concentrated luminosity. The galaxy displays variations in color across its structure. The central bulge exhibits a redder hue, possibly indicative of an older stellar population. The spiral arms show patches of bluer color, likely associated with regions of ongoing star formation where younger, hotter stars reside. Overall, the galaxy is of intermediate size.
