The galaxy presents as a centrally concentrated object with a smooth overall appearance. The core region exhibits a bright, compact morphology, suggesting a high density of stars and potentially the presence of an active galactic nucleus, or a supermassive black hole. 

Moving outwards from the core, the light distribution fades gradually into a more diffuse halo or disk component. There are hints of possible faint, disturbed features or tidal tails, suggesting some sort of gravitational interaction event in the past.

The color distribution within the galaxy is not uniform. The central region appears to be dominated by bluer wavelengths. The outer regions appear dominated by greener wavelengths.
