The galaxy exhibits a morphology suggestive of a late-stage merger or significant interaction. The primary body of the galaxy appears somewhat amorphous, displaying a centrally concentrated luminosity profile with a smooth overall appearance. Evidence of tidal features or extended stellar envelopes is visible, potentially indicating past or ongoing gravitational interactions. The color gradient suggests a relatively evolved stellar population, with a dominant reddish-yellow hue. The galaxy has a large mass and is possibly forming stars at a low rate. This galaxy appears to be the product of a merger event between multiple galaxies.
