This galaxy presents as a smooth, elongated object, likely an elliptical galaxy viewed at an oblique angle. The central region exhibits a concentrated, bright, yellowish hue, suggesting an older stellar population dominating the core. Fainter, diffuse light extends outwards from the central bulge, creating a cigar-shaped profile. The outer regions appear less defined, with a gradual decrease in luminosity as the galaxy blends into the background. There is no discernible spiral structure or prominent dust lanes visible, supporting the classification as an elliptical galaxy. There may be some minor tidal disturbances. The overall morphology points to a gravitationally relaxed system with a relatively low star formation rate.