The galaxy presents as a moderately inclined, disk-shaped structure. It exhibits a central bulge which is not especially prominent. The disk appears somewhat irregular, hinting at possible past interactions or internal disturbances. Within the disk, we observe a mottled texture, possibly indicating regions of star formation. The color is distinctly blue, suggesting a population of young, hot stars. The galaxy appears relatively isolated with no obvious major merger occurring. The overall morphology suggests a late-type spiral galaxy, with ongoing, albeit not extremely vigorous, star formation. Its overall appearance is slightly disturbed, but not exceptionally so.
