The galaxy presents a prominent disk structure, oriented at a slight angle to our line of sight. Spiral arms are clearly discernible, exhibiting a tightly wound morphology. I estimate three distinct spiral arms, though some asymmetry is evident in their structure and definition. A central bulge is present, of moderate size, and appears relatively bright. There is no evidence to suggest a strong bar feature. The disk shows evidence of ongoing star formation, as inferred from the slightly blueish hue. There appears to be no current merger activity disrupting the overall morphology.
