The galaxy presents an overall spiral morphology, though some disk structures are not as clear and defined as in more typical examples. The central bulge is prominent and appears moderately sized compared to the rest of the galaxy, exhibiting a yellowish-white hue, suggestive of an older stellar population. Fainter, diffuse spiral arms emanate from the central bulge, showing hints of bluer regions. The galaxy's disk appears mostly face-on with no disturbances. There is no obvious sign of a stellar bar structure. The spiral arms are not very tightly wound and appear somewhat patchy. 