The galaxy presents an elliptical morphology, with a smooth light distribution lacking any apparent spiral arms or significant dust lanes. The core is highly luminous, exhibiting a concentrated and bright central region. Moving outwards, the galaxy gradually fades into the background sky, with no sharp edges observed. There is some evidence of interaction or past merger event given the distorted shape and possible faint tidal tail extending from the galaxy. There are slight indications of possible ongoing mergers due to the asymmetrical shape of the galaxy, with one side appearing more elongated. The overall color profile suggests an older stellar population, exhibiting a reddish-yellow hue that indicates a predominance of evolved stars and a relatively low rate of current star formation. The galaxy appears to be massive, given its considerable size and luminosity.
