The galaxy presents as an elongated, ellipsoidal structure. Its central region exhibits a high degree of luminosity, suggestive of a concentrated stellar population or active galactic nucleus. The overall color profile trends towards redder wavelengths, particularly within the core. This indicates a dominance of older stellar populations and/or significant dust obscuration. The outer regions of the galaxy show a more diffuse distribution of light, with a gradual decrease in surface brightness from the core. There is little visible evidence of spiral arm structure or prominent star-forming regions. The galaxy's shape is somewhat irregular. It does not appear to be undergoing a major merger, although there is a slight asymmetry that warrants further investigation. The galaxy's smooth light distribution indicates that it is likely to be relatively evolved, with star formation having largely subsided. The approximate physical extent is estimated to be 8 kpc. 
