The galaxy presents a generally amorphous shape. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars and potentially an active galactic nucleus. Faint extensions of light emanate from the central region, indicating a diffuse halo or possible tidal features. A slight asymmetry is noticeable in the outer regions, potentially suggestive of gravitational interaction or recent merger activity. The overall color profile indicates a mix of stellar populations with some regions displaying bluer hues which could be indicative of ongoing star formation, and other parts redder indicating a more mature population of stars. 
