The galaxy appears as a relatively compact object with a centrally concentrated light profile. The overall form exhibits a degree of irregularity, suggesting a potential non-equilibrium state.

The core region is bright and unresolved, possibly indicating the presence of an active galactic nucleus or a dense concentration of stars. Surrounding this core is a more diffuse halo of light that appears to be asymmetric. Patches of bluer light are visible towards the outer edges, which may indicate regions of recent or ongoing star formation. 

There is evidence of possible tidal features or distortions extending outwards from the main body of the galaxy, suggesting a potential recent or ongoing interaction or merger event. The overall color gradient suggests an older stellar population in the core, surrounded by younger, bluer stars in the outer regions.
