The galaxy presents an irregular morphology, appearing as a somewhat amorphous central bulge. Its color profile indicates a generally older stellar population with a redder hue overall, most strongly in the central region. There are noticeable disturbances in the shape, possibly indicating tidal interactions. Two distinct components exist, suggesting a galaxy merger event in progress. There is an absence of clearly defined spiral arms or a distinct disk structure and a dominant, smooth feature, lending to the appearance of an elliptical type of galaxy.
