The galaxy presents as a centrally concentrated system, characterized by a smooth and relatively featureless morphology. Its overall shape approximates an ellipse, exhibiting an intermediate degree of ellipticity. The dominant color is yellowish, with a slight reddening gradient visible toward the core. There is some visual evidence that the galaxy may be interacting or merging with a nearby object, as there are some distortions on one side of the galaxy.

The absence of clearly defined spiral arms or prominent dust lanes suggests that it is unlikely to be a spiral galaxy and is likely to be either an elliptical galaxy or a lenticular galaxy. The color suggests an older stellar population and/or a significant amount of dust, which is consistent with a relatively low rate of star formation. Overall, the appearance of the galaxy indicates that it is an evolved system, possibly transitioning towards a more passive state.
