The galaxy appears as a centrally concentrated object with a somewhat indistinct morphology. There is no clear spiral arm structure visible. It exhibits a color gradient, transitioning from a more bluish hue in the central region to redder tones in the outer portions. The relative smoothness of the galaxy suggests that it could be an elliptical galaxy, although some disk-like features might also be present. The apparent lack of defined structure could also indicate that the galaxy is undergoing a merger event, causing a disruption of its original morphology. There may be faint tidal features visible, which lends some support to it being in the late stages of a merger. The estimated size and inferred mass appear typical for galaxies in the local universe. There is evidence of ongoing star formation, at an intermediate rate.
