The galaxy presents as a relatively smooth, elliptical-like object. There is an amorphous central bulge that appears slightly elongated along the vertical axis. A significant fraction of the galaxy's light is concentrated in this central region, suggesting a high stellar density. The overall color appears yellowish, indicative of an older stellar population with relatively low levels of ongoing star formation. Some light disturbances are apparent, and the possibility of an ongoing merger cannot be discounted. However, there is no tidal tail or obvious sign of interactions with other galaxies. The outskirts are unresolved, fading gradually into the background sky.
