The galaxy presents as a single, dominant, relatively smooth and rounded object. There appears to be some minor morphological disturbance to one side of the galaxy, though it is not clear whether this is an interaction or internal process. The color profile of the galaxy is relatively consistent throughout, with a slightly redder hue. This red color suggests an older stellar population and/or significant dust obscuration, and implies a suppressed star formation rate. The galaxy's roundness suggests it is likely an elliptical galaxy. The overall appearance suggests a mature galaxy, potentially a large elliptical galaxy.
