The galaxy presents a somewhat elliptical morphology, appearing as a smooth concentration of light with a central bulge that is relatively prominent. The galaxy's light distribution transitions smoothly from the core to its outer regions without any distinct spiral arm structures visible in this image. The galaxy appears to be moderately elongated. There are hints of subtle dust lanes or features, but overall the galaxy appears relatively undisturbed, without any obvious signs of a recent major merger. The galaxy has an intermediate color, suggesting a mix of stellar populations, neither strongly blue, indicative of intense recent star formation, nor extremely red, suggesting an aging population of stars.
