The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. Its central bulge appears prominent and concentrated, emitting a strong blue-white light, suggestive of a population of hot, young stars. The disk exhibits a less intense blue color, indicative of ongoing star formation. The overall shape is moderately elongated, but mostly between cigar shaped and round. There may be slight disturbances along the edges of the galaxy, possibly due to minor gravitational interactions or internal processes. No clear spiral arm structure or distinct dust lanes are discernible in this image.
