The galaxy presents as a moderately inclined spiral with a prominent disk. Two distinct spiral arms are readily visible, tracing a clear pattern from the central region outwards. The winding of the spiral arms appears to be primarily of medium tightness. There's a noticeable central bulge of moderate size. A weak bar structure seems to be present, extending across the galaxy's nucleus. The overall structure shows no significant signs of major disruption or ongoing merging activity, although there may be hints of minor disturbances. Dust lanes appear within the spiral arms, contributing to the patchy appearance. The galaxy exhibits a blue hue, suggesting active star formation.
