The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse light profile, with a notable absence of distinct spiral arms or prominent dust lanes. The galaxy's core appears bright, suggesting a dense population of stars in the central region. The overall color appears yellowish-red, which indicates an older stellar population and a relatively low rate of ongoing star formation. There is a subtle extension of light outward from the central region, which is a possible extended stellar halo or tidal features resulting from a past interaction, although the image quality makes it difficult to confirm. No signs of significant morphological disturbance, like tidal tails or obvious merger remnants, are apparent in the image, suggesting it is a relatively settled system.
