The galaxy presents an elliptical morphology, appearing largely spheroidal with a smooth light distribution and a slight elongation. The central region exhibits a concentration of light, with a gradual decrease in intensity towards the outer edges. The galaxy's color profile is generally uniform, with subtle variations across its surface. There are no readily apparent spiral arms or dust lanes within the galaxy. A potential minor disturbance is visible in the form of slight asymmetry. There is an indication of a merger event, but if a merger did occur, it appears to be in its late stage.
