The galaxy appears as a single, somewhat amorphous structure, but is likely undergoing a significant merger event, possibly involving two or more galaxies. There is some evidence for minor disturbances in the morphology, indicating ongoing gravitational interactions. The central region is dominated by older stellar populations, exhibiting a yellowish-red hue. Evidence shows that it may be actively forming stars, although at a relatively low rate. The galaxy exhibits an overall smooth appearance. There are no distinctly defined spiral arms or a prominent disk component visible. The overall shape is elliptical.
