The galaxy presents as a spiral type, exhibiting a disk-like morphology. Prominent spiral arms are visible, appearing loosely wound. Two main arms are discernible. A central bulge is present; it appears to be moderate in size, but it is difficult to say for sure with the orientation and image quality. The galaxy displays an overall bluish tint in its arms, indicative of ongoing star formation. There is no evidence of a strong bar structure. The galaxy's disk shows a slight inclination relative to the line of sight, but is not quite edge-on. There does not seem to be any major interaction or merging with nearby galaxies; however, there is possible minor disturbance in the arms. The galaxy's luminosity appears moderate, suggesting a relatively active stellar population.
