The galaxy presents as a relatively compact object with a generally smooth profile. It appears to be an elliptical galaxy, though it may have a weak disk component. The core of the galaxy is fairly luminous. The galaxy exhibits a color gradient, with the central region appearing to be of a yellowish-orange hue, transitioning to a bluer color in the outer regions. This may indicate ongoing or recent star formation. There is no evidence of a strong spiral arm structure. No signs of a major merger can be observed. There might be evidence of tidal disturbances or minor interactions.