The galaxy appears to be a spiral galaxy exhibiting a well-defined disk structure. The spiral arms are prominent, displaying a relatively open morphology. A central bulge is visible, contributing significantly to the galaxy's overall luminosity, though not necessarily dominant. The disk appears to be viewed at a slight angle, but is still relatively face-on. There is no strong evidence of a prominent bar structure, but a subtle central elongation might suggest a weak bar. The galaxy shows indications of ongoing star formation, particularly within the spiral arms, as suggested by their somewhat patchy appearance and hints of bluer color. No apparent major merging or significant tidal disturbances were seen in the structure of the galaxy.
