The galaxy presents as a spiral with a predominantly blue hue, indicating a substantial population of young, hot stars and ongoing star formation. The spiral arms are well-defined, exhibiting a multi-armed structure, most likely two, and a moderately wound morphology. There appears to be a faint central bulge of moderate size, and no sign of a central bar. The overall form displays some irregularities, potentially suggesting minor gravitational interaction or internal disturbances. There is no evidence of a recent major merger.
