The galaxy presents as an elongated, lenticular object, possibly an elliptical galaxy seen at an angle. Its core is a bright, concentrated region, appearing yellowish-white, suggesting a population of older stars. The light becomes more diffuse as it extends outwards from the center. The galaxy is surrounded by a fainter halo of light that shows signs of a disk-like structure. There are no well-defined spiral arms or dust lanes visible. The morphology suggests it is a relatively evolved system that appears smooth. There is a very faint hint of possible tidal interactions on the outer edges, which would merit further investigation. Overall, it is characterized by a high Sersic index indicating that its light profile is centrally concentrated.
