The galaxy presents as a relatively bright object, exhibiting a smooth, elliptical morphology. There's a primary core that appears quite concentrated and luminous. A fainter secondary core is also visible to the right, and seems to be interacting with the primary core. The overall color profile suggests a population dominated by older stars. The outer regions fade gradually without distinct spiral arms or prominent dust lanes. There are faint traces of ongoing star formation, indicated by bluer emissions in areas surrounding the center. There are signs of a major merging event affecting the structure of the object.
