The galaxy presents a largely smooth, elliptical morphology. There is a bright central bulge, potentially indicative of a supermassive black hole. The light distribution suggests a relatively even stellar population, with little evidence of prominent spiral arms or dust lanes. The galaxy displays a somewhat round shape, with a slight elongation. There is no clear indication of ongoing major merging events. The galaxy appears to be a relatively isolated system, with a hint of some minor disturbance. The overall color profile suggests a mix of stellar populations, with a tendency towards older, redder stars.
