The galaxy presents as a slightly elongated, disk-like structure. A central bulge appears prominent, exhibiting a smoother, more concentrated light distribution. The overall color suggests a relatively mature stellar population.

The disk component is faintly visible, extending outwards from the bulge with hints of spiral structure. There may be some evidence of ongoing star formation within these arms.

The system exhibits a possible tidal tail or minor merging disturbance to one side. The primary body of the galaxy appears relatively undisturbed.
