The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a high degree of luminosity, indicating a concentration of stars. The galaxy appears to have a central bulge. Extending from the central region, one arm is visible. This arm appears bluer in color, suggesting younger stellar populations and potential ongoing star formation. The other arm is less visible. The overall structure of the galaxy does not exhibit clear spiral arm morphology, and may have some disturbances. There are no obvious signs of a major merger.
