The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears a yellowish-white hue. The galaxy fades gradually toward its edges, lacking sharp boundaries, which suggests a diffuse halo surrounding the brighter central region. The overall shape is elongated, indicating a possible elliptical morphology rather than a spiral. There is very little discernible internal structure such as spiral arms or dust lanes. The galaxy is generally isolated with no obvious signs of interaction with nearby galaxies. The even color and smooth texture may suggest a relatively older stellar population and lower current star formation rate.
