The galaxy exhibits a roughly elliptical morphology, appearing significantly elongated along a single axis. A bright, concentrated central bulge region is clearly visible, indicating a high stellar density core. The surrounding galactic disc shows some evidence of structure, but lacks well-defined spiral arms. A faint, diffuse halo extends beyond the main body of the galaxy. Color gradients are apparent, with the central bulge exhibiting a brighter white hue and the outer regions of the disc showing hints of bluer colors. Possible tidal disturbances or faint plumes emanate outwards. These faint structures could suggest a history of minor mergers or interactions with smaller companion galaxies.
