This galaxy presents as an elongated, disk-like structure, exhibiting a moderate level of smoothness in its overall form. The light distribution suggests a concentration towards the central region, with a gradual decrease in brightness towards the outer edges. While the dominant color is a warm, yellowish-white, subtle variations in hue are present, hinting at underlying structural components and differing stellar populations. The galaxy's shape implies a potential elliptical morphology, but it could also be a spiral galaxy viewed edge-on. There is no visually prominent evidence of ongoing merging activity or major disturbances in its structure. The object appears relatively isolated, showing no obvious signs of close interaction with neighboring galaxies. The apparent size is small, suggesting a significant distance.
