The galaxy appears to be elliptical in shape, with a smooth, relatively featureless morphology. The central region exhibits a concentrated, bright core, transitioning to a fainter, more diffuse halo. The color gradient suggests an older stellar population, with a reddish hue in the core possibly indicating a higher concentration of older, cooler stars. Hints of blue around the outside edges of the galaxy may indicate a very small presence of younger stars. There is little evidence of spiral arms or significant dust lanes. It is fairly isolated. Overall, the galaxy appears to be a fairly typical example of an elliptical galaxy, possibly in a late stage of its evolution.
