This galaxy exhibits a morphology that suggests it is a spiral galaxy, presenting a disk-like structure. The galaxy does not appear to be edge-on, but is tilted slightly. Within the galaxy, spiral arms are faintly visible, with a moderate bulge, not entirely dominant but neither particularly small, is observed. It has neither a strong or weak bar. Indications of some disturbances, potentially due to minor interactions, may be present, though a major merger does not seem likely. Overall, the galaxy shows signs of some star formation activity, not particularly quiescent, but not extremely vigorous either. The galaxy's structure is dominated by its spiral arms, and it is likely classified as a galaxy with features or a disk. The general color suggests a mix of stellar populations, and the galaxy does not appear to be a purely elliptical or smooth galaxy.