The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. Its color appears predominantly yellow-orange, suggesting an older stellar population with diminished ongoing star formation. The light distribution indicates a centrally dominant luminosity, with a gradual decrease in surface brightness outwards. There are no clearly defined spiral arms or distinct dust lanes visible. Some irregularities in the light distribution indicate a possible interaction or minor disturbance occurring. There are also a few bright spots within the galaxy that could possibly be star forming areas. The overall form suggests a system that has undergone significant dynamical relaxation.
