The galaxy presents as a diffuse, elongated structure, appearing cigar-shaped in its overall morphology. The central region is characterized by a bright, concentrated luminosity, indicative of a dense stellar population and/or active galactic nucleus. The outer regions exhibit a smoother texture with a gradual decrease in luminosity towards the edges, possibly caused by the dust. Faint blue features can be observed in the extremities of the galaxy, indicating that there may be lower levels of star formation in these regions. The overall structure lacks any prominent spiral arms or disk-like features, suggesting that it is not a spiral galaxy. There are no signs of ongoing major mergers or significant tidal disturbances. The galaxy is likely an elliptical galaxy.
