The galaxy presents as an elliptical morphology, with a generally smooth appearance. It exhibits a bright central bulge that fades gradually outward, with no distinct spiral arms or bar structure visible. The overall color profile appears slightly redder, with the core being the reddest part of the galaxy. There is a very faint suggestion of a possible disk or flattening, but this is difficult to assess due to the low resolution. No apparent signs of active galactic nuclei or strong star formation regions are immediately obvious based on the observed light. There is a very slight suggestion of a minor disturbance in the galaxy's shape, but not an ongoing merger event.