The galaxy presents as a centrally concentrated elliptical-like structure. The core region exhibits a reddish hue, potentially indicating an older stellar population or significant dust obscuration. Surrounding the core, a more diffuse greenish-yellow halo extends outwards. This suggests the presence of a younger stellar population or ongoing star formation in the outer regions, albeit at a lower rate compared to galaxies actively undergoing intense starburst activity. The overall morphology appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The galaxy's light distribution is largely smooth, with only subtle variations in color and intensity across its surface. Its shape appears roughly elliptical, leaning more towards the 'in between' area between fully round and slightly flattened. There is an indication of a possible minor disturbance in the galaxy's halo. Overall, this galaxy appears to be a moderately massive system with a mix of stellar populations, with no intense star forming activity or tidal disturbances.
