The galaxy appears to be largely smooth in overall texture. It exhibits an elliptical morphology, appearing elongated with a high degree of cigar shape. There is a subtle color gradient across the galaxy, transitioning from a bluer hue on one end to a redder hue on the other. This suggests a potential difference in stellar populations or dust content across the galaxy. There are no obvious signs of spiral arm structure or a prominent disk. It shows little indication of any recent major merger activity or significant tidal disturbances. The light is centrally concentrated, with a gradual decrease in luminosity moving outward from the core.
