The observed galaxy presents a prominent, albeit somewhat indistinct, spiral structure. The arms appear tightly wound and display a fuzzy morphology, indicating possible significant dust obscuration or active star formation regions. The spiral arms seem to be somewhat difficult to resolve individually, possibly due to an inclination angle that is somewhat edge-on.

A bright central bulge dominates the galaxy's core, exhibiting a yellowish hue. This color suggests an older stellar population residing in the bulge. The surrounding disk shows a bluer tinge in the areas between the arms. There appears to be no prominent bar structure. There may be minor disturbances indicating gravitational interactions with other galaxies. 
