The galaxy presents a largely smooth morphology, with a high degree of central concentration. The light profile indicates that this galaxy is elliptical in nature, exhibiting a spheroidal structure without apparent spiral arms or a distinct disk. The core region displays a notably redder color, suggesting an older stellar population dominated by evolved stars and a lower rate of current star formation. The outer regions transition to slightly bluer hues, hinting at some residual or recent star formation activity, although at a much lower level compared to the central region. The galaxy appears relatively undisturbed, lacking any strong visual evidence of recent major mergers or tidal interactions. There are some possible minor disturbances observable. The overall shape appears rounded and the mass of the galaxy is substantial. 
