The galaxy appears as a relatively compact object. Morphologically, it presents as an elliptical galaxy based on the image. There are two distinct bright regions visible, appearing to be two interacting galaxies merging to form a single object. There are no obvious spiral arms or a well-defined disk structure. The galaxy has a color gradient, appearing bluer in the central regions, becoming progressively redder outwards. There is some visual evidence of a tidal tail or disrupted features, indicative of gravitational interactions. Overall, the galaxy displays characteristics consistent with an ongoing galaxy merger event.
