This galaxy appears to be an elliptical-type galaxy, with a smooth, largely featureless appearance. It presents as a concentrated central bulge that fades into an extended halo of light. The shape of the galaxy is generally round. A slight asymmetry or disturbance is visible, possibly indicative of a recent minor merger or tidal interaction. There is a possibility of ongoing star formation, as evidenced by slight variations in color across the galaxy's body, although this may also be due to dust or varying stellar populations. Overall, the galaxy seems to be at an intermediate stage in its evolution, possibly transitioning from a more active to a passive state.
