The galaxy presents as a lenticular or early-type spiral with a notably smooth and concentrated central bulge, elongated in shape. There is an absence of clearly defined spiral arms or prominent dust lanes. The overall color profile appears slightly reddish-yellow, with a more pronounced yellow hue towards the core. This color suggests a stellar population that is relatively old and metal-rich. The galaxy is likely massive, and it has a low rate of star formation. The regular morphology indicates it is not undergoing a major merger, although there is potential for minor disturbances or interactions in its past.
