The galaxy presents as a relatively compact object with a subtly elongated shape. It exhibits a relatively smooth profile, with minimal indication of spiral arms or significant substructure. The central region appears slightly brighter. There seems to be a suggestion of minor tidal disturbance or asymmetry within the galaxy's outer regions, but further investigation is needed to ascertain the nature and extent of this possible disturbance. Integrated light suggests that it is brightest in the green and red regions.