The galaxy presents as a relatively smooth, elliptical-like structure. There is little evidence of spiral arms or a prominent disk. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer edges. The galaxy exhibits a yellowish-orange hue, which could indicate an older stellar population. The overall shape is roughly circular, although a subtle elongation is potentially present. No obvious signs of active galactic nuclei, dust lanes, or ongoing star formation are immediately discernible from the image. There are no tidal tails or clear signs of major mergers in its recent history. Minor disturbances may be present but difficult to assert.
