The galaxy presents as a relatively compact, disk-shaped system, seen at a significant inclination. The central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk component displays a bluer color gradient from the bulge outwards indicating the presence of younger stars, and potential ongoing star formation. There is a slight asymmetry in the outer regions of the disk, possibly indicating a minor gravitational interaction or disturbance. The overall structure is generally smooth, lacking clear spiral arm definition within the observable range.
