The galaxy appears as an elliptical morphology. It presents a smooth, concentrated light profile, with no discernible spiral arm structure or prominent dust lanes visible in this image. The galaxy has a slightly elongated shape, with an approximate ratio of minor to major axis of maybe 2:3. A color gradient is observed, with a more yellowish hue concentrated towards the central region, indicating a possibly older stellar population in the bulge. The outer regions appear slightly bluer, suggesting the presence of some younger stars. Overall, the galaxy seems to be a relatively undisturbed, evolved system.
