The galaxy presents a somewhat elongated, cigar-shaped morphology. The central bulge region appears relatively smooth and concentrated, exhibiting a bright core. A disk component is visible, though it is not particularly well-defined or prominent. There are hints of some disturbances within the disk, potentially indicative of minor gravitational interactions or internal activity. Based on the general shape and structure, it may be classified as an intermediate-type galaxy, possibly an Sa or Sb spiral, seen at an oblique angle. The light from the disk appears slightly bluer than that from the bulge, suggesting some ongoing star formation within the disk. The red shift indicates the galaxy is a considerable distance away. Overall, the galaxy seems to be of moderate size and mass.
