The galaxy presents a mostly smooth, elliptical morphology. Its light profile appears largely featureless, with a concentration of light towards the center. The color index suggests a relatively older stellar population, with the light tending towards the redder end of the spectrum. While largely appearing as a single system, there is potentially some very subtle indication of minor tidal disturbance in its outer reaches. No clear spiral arms or significant dust lanes are apparent. The overall roundness suggests it is closer to an elliptical galaxy than a highly flattened spiral.
