The galaxy presents as a spiral type, exhibiting a generally face-on orientation relative to our line of sight. The arms are somewhat distinct. The central bulge appears bright and concentrated with some evidence of possible disk structure. There is a suggestion of spiral arm structure emanating from the core region, with a flocculent appearance. There is some possible minor disturbance. Overall, the galaxy has a notable spiral structure, though not perfectly symmetrical, with indications of ongoing star formation.
