The galaxy presents a generally elongated, spindle-like morphology. The central region exhibits a concentrated luminosity profile, appearing relatively smooth and featureless. Moving outward from the core, the luminosity gradually decreases. There is a disk-like structure component, as evidenced by the relatively narrow major axis. The light distribution suggests an older stellar population, with a redder color. There is no apparent bulge. Faint features or irregularities are present on the outer edges that could potentially indicate tidal interactions or disturbances.
