The galaxy presents a generally smooth appearance, but with some visible features. The central region is bright and concentrated, with a yellowish hue indicating an older stellar population. Moving outwards, a flattened disk-like structure can be observed, oriented at an angle to our line of sight. There is some evidence of substructure within the disk, but details are unclear from the resolution. One side of the galaxy appears more disturbed than the other, with a slight extension or tidal feature possibly indicating an interaction with a smaller galaxy, or some other minor gravitational disturbance. Star formation appears low, based on its red color. The overall shape of the galaxy is intermediate between a flattened disk and a more spherical shape, suggesting it is not a pure elliptical or spiral, but likely an intermediate galaxy type.
