The galaxy presents as a faint, irregular spiral structure. A prominent disk is visible, oriented at an angle that allows for a clear view of spiral arm features. The arms are somewhat patchy and not clearly defined, exhibiting a flocculent morphology with areas of clumpy star formation. There appears to be a small central bulge, but it is not very pronounced. No strong bar structure is apparent. There is evidence of minor gravitational disturbance or interaction, as indicated by the slightly distorted shape of the spiral arms. Overall, the galaxy exhibits a blueish hue, suggesting a relatively young stellar population and ongoing star formation within the disk.
