The galaxy exhibits a defined central bulge which is moderately bright and appears to be somewhat spheroidal in shape. Surrounding the bulge, there is a visible disk structure. The galaxy appears inclined to our line of sight, showing an elliptical projection. The disk presents with broad, indistinct spiral arm features, exhibiting a patchy texture that indicates regions of star formation or dust obscuration within the disk. The overall color of the galaxy is slightly reddish, possibly indicating an older stellar population. The galaxy is not undergoing any major mergers, though a minor disturbance may be present. There is a hint of a weak bar structure within the central region. The outer edges of the disk fade into the background, suggesting a gradual decrease in stellar density.
