The galaxy presents as a spiral morphology, characterized by a prominent central bulge that appears moderately bright and yellowish in color. Two well-defined spiral arms emanate from this central region. The arms exhibit a relatively tight winding pattern. Star formation is evident within the arms, manifested as localized bluish regions indicative of younger, hotter stellar populations. There is no obvious bar structure apparent in the galaxy's central region. The galaxy does not appear to be strongly interacting or merging with other galaxies based on the image; however, there are small disturbances present.
