The galaxy presents a disk-like morphology, oriented at a moderate inclination relative to our line of sight. A central bulge is discernable with a yellowish hue, suggesting an older stellar population. Extending from the bulge, the disk shows evidence of spiral arm structure, though somewhat flocculent. The arms exhibit a bluer color, indicative of ongoing star formation. The overall shape is somewhat irregular and there is a slight distortion in one of the spiral arms, possibly hinting at a minor gravitational interaction. There is low level, widespread star formation.
