The galaxy presents an elongated, elliptical morphology. It displays a relatively smooth texture, suggesting a lack of significant spiral arm structure. The light distribution appears concentrated towards the center, indicating a bulge-dominated system. There is an observed color gradient, with the central region appearing more yellow-orange in hue, transitioning to a slightly bluer color in the outer regions. This could be indicative of older stellar populations concentrated towards the center. There are some possible faint features or disturbances in the galaxy's outskirts, possibly faint tidal tails or remnants of a minor merger event. The general structure does not appear highly disturbed, suggesting that any potential merger activity is in a relatively late stage.
