The galaxy appears as a somewhat diffuse object with an overall elliptical morphology, though not perfectly circular. It presents a bright, concentrated central region, likely indicating a significant stellar population and potentially a supermassive black hole. The central region transitions smoothly outward, fading into a less dense halo. The galaxy exhibits a subtle bluish hue, potentially suggesting ongoing star formation, or a population of hot, young stars. There are some minor disturbances in the outer regions, with some hints of a possible interaction or past merger event. Overall, the galaxy presents a blend of smooth features, with some subtle indications of dynamic processes.