This galaxy exhibits a spiral structure, characterized by prominent spiral arms extending from a central bulge. The arms are not tightly wound, indicating a later Hubble type classification. Star formation appears active, with bluish hues visible along the spiral arms, suggesting the presence of young, hot stars. The bulge is moderately sized. The galaxy presents a disk-like appearance. There is no evidence of significant tidal distortions or ongoing major merger activity; however, the morphology does suggest some possible minor interaction or internal disturbance. A bar-like structure may be present, bisecting the central bulge.
