The galaxy presents as a dual system, comprised of two distinct components with evidence suggesting an ongoing interaction or merger. The primary galaxy appears as a large, relatively featureless elliptical galaxy, exhibiting a smooth light distribution characterized by a concentrated central bulge. Its overall color is slightly yellow, indicating an older stellar population and suppressed recent star formation.

The secondary component displays a more disturbed morphology, with an irregular shape and a hint of tidal features possibly indicating ongoing gravitational disruption. Its color appears slightly bluer than the primary, potentially suggesting the presence of younger stars. The spatial proximity and morphological disturbances suggest a possible ongoing interaction with the primary galaxy which may be a minor merger.

The overall system appears to be in a relatively quiescent state regarding star formation, although the secondary component appears slightly more active. The interaction between the two galaxies may be influencing their star formation rates.
