The galaxy presents as a single, concentrated luminous core surrounded by a diffuse, extended halo. The core exhibits a smooth, centrally-peaked light distribution, indicative of an older stellar population. The halo lacks any readily discernible spiral arm structures or distinct features. It shows a slight flattening. Overall the galaxy is a bright, elliptical or lenticular morphology with no signs of strong star formation. There is no apparent tidal disturbance or interaction with neighboring objects.
