The galaxy presents as a spiral type, exhibiting a prominent disk structure. The galaxy is not viewed edge-on, but rather at a noticeable angle which reveals arm structure. The arms are tightly wound. A central bulge is evident, though moderate in size relative to the galactic disk. The central region appears yellowish, suggesting an older stellar population, while the outer regions of the disk exhibit a bluer hue, indicative of ongoing star formation. The overall morphology suggests the presence of a bar structure. There is no immediately apparent indication of any major mergers or significant tidal disturbances.
