The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution is generally even, with a noticeable decrease in intensity moving outward from the center. There is a hint of a disk or slightly flattened shape, but the overall form is primarily spheroidal. The galaxy's color profile suggests it is a mature system with an older stellar population, based on the redder hues observed. There may be some minor disturbances within the galaxy, possibly indicative of past interaction with another galaxy. Overall, the galaxy presents as a massive, quiescent system.
