The galaxy presents as a smooth, elongated structure with a high degree of ellipticity. Its overall color profile is a mix of light blues and yellows. The light blue hue is located mostly towards the center of the galaxy. These may indicate varying stellar populations or dust content. The light distribution appears relatively uniform across the galaxy, without prominent spiral arm structures or a distinct bulge component. There are no obvious signs of recent major merger activity or tidal distortions in its morphology, with perhaps some minor disturbances. Its smooth appearance suggests a potentially evolved stellar population with a lower rate of ongoing star formation. The size is moderately small.
