The galaxy appears as a binary system, consisting of two distinct components.

The first component is a relatively compact and smooth elliptical galaxy, exhibiting a bluish-white hue. Its shape is roughly intermediate between circular and elongated. There is no visible indication of a prominent disk or spiral arm structures.

The second component is similarly smooth and compact, with a yellowish-orange color profile. It presents a similar intermediate shape between circular and elongated, akin to the first component, but the color suggests an older stellar population.

There is no clear evidence of substantial tidal distortion or merging activity, although subtle disturbances may be present. The overall structure of both components seems relatively relaxed and undisturbed.
