The galaxy exhibits a generally elliptical morphology. Its light profile appears relatively smooth, without pronounced spiral arm structures or distinct dust lanes visible in this image. The core region presents a concentrated brightness, suggesting a significant stellar population density. There is a slight elongation observed, indicating it's not perfectly spherical. The color appears yellow/white indicating likely older stellar populations with few younger blue stars. Overall, the galaxy seems to be a massive system with relatively low ongoing star formation. Faint hints of tidal disturbances or interactions are observable, indicating a possible merger event.
