The galaxy presents as a single, relatively symmetrical object with a smooth, concentrated light profile. The galaxy's overall color is a yellowish-white hue, suggesting an older stellar population. The light is centrally concentrated, with a gradual decrease in intensity toward the outer regions. There is a slight elongation and possible disturbance of a minor nature. No distinct spiral arms or bar structures are discernible, indicating a likely elliptical or lenticular morphology. There is the potential of this galaxy being in the midst of a merging event.
