The galaxy presents a flattened, elliptical shape with a discernible disk structure. A pronounced central bulge is observed, appearing relatively smooth and bright. The color gradient shifts from a bluer hue at the center of the disk to a redder tint towards the outer regions, possibly indicative of varying stellar populations or dust distribution. The disk appears to be tilted relative to the line of sight. There is some indication of irregularities in the outer disk regions which could indicate a small disturbance or an interaction with a companion galaxy. The overall structure suggests a relatively mature galaxy, yet not entirely undisturbed, showing hints of recent, minor interaction with other galactic body.
