The galaxy presents as a somewhat elongated, lenticular or early-type spiral galaxy. Its central bulge appears prominent and smooth, displaying a concentrated luminosity profile. The overall color suggests an older stellar population, with a lack of significant blue light indicative of active, ongoing star formation. There is no obvious dust lane visible. There seems to be a very slight flattening suggesting a disk, but the object is primarily smooth and ellipsoidal in appearance, lacking any prominent spiral arm structures. The morphology is relatively undisturbed, showing no strong signs of recent major merger activity, although some minor irregularities in the outer regions cannot be ruled out. The object seems to be neither perfectly round nor highly elongated; rather, it exists in an intermediate state.
