The galaxy presents as a somewhat elongated object with a core region that appears relatively smooth and concentrated. The central region exhibits a cyan hue, possibly indicating a population of young, hot stars or active galactic nucleus activity, though higher resolution imaging would be required to confirm. Extending outwards from the core is a more diffuse structure, displaying a reddish-yellow gradient that may suggest a distribution of older stellar populations or dust obscuration.

The overall form suggests a potential ongoing merger or tidal interaction, as the shape deviates significantly from a perfect elliptical form. There appears to be a faint extension or tidal tail emanating from the core region, further hinting at gravitational disturbance. This galaxy appears relatively massive, based on its considerable luminosity and extended structure.

The apparent smoothness of the central region suggests that it might be an early type galaxy (Elliptical or lenticular), however the tidal tail indicates a very late merger that is causing star formation in the centre, so it might be an active spiral galaxy.
