The galaxy presents a reddish-orange hue, indicative of an older stellar population and dust obscuration. Its morphology appears to be undergoing a significant interaction, possibly a merger event, as evidenced by the distorted shape and possible presence of tidal features. There is an irregular shape, with a brighter central region, which may host an active galactic nucleus (AGN). Based on the color and morphological irregularities, this galaxy has a low rate of star formation. The galaxy's luminosity suggests it's a massive system.
