The galaxy presents an elongated, cigar-like morphology. It appears relatively smooth in structure, lacking prominent spiral arms or significant dust lanes. A central bulge is visible, exhibiting a yellowish hue suggesting an older stellar population. The light diminishes towards the outer edges of the galaxy, indicating a decreasing density of stars. There is a slight bluer tone surrounding the central yellowish bulge, which may indicate recent star formation. There is no evidence of an active galactic nucleus or any significant tidal disturbances to suggest a recent merger event. The overall shape and color suggest an elliptical-like galaxy that is far from the observer.
