The galaxy presents an overall elliptical morphology, appearing somewhat flattened. The light profile seems centrally concentrated, with a smooth, diffuse glow emanating outwards. There is a subtle hint of disk-like structure, but it is not sharply defined. A distinct color gradient is observable; the core appears more yellow, potentially indicating an older stellar population, while the outer regions have a slightly bluer hue, possibly due to the presence of younger, hotter stars or ongoing star formation, albeit at a modest rate.  There is a possible interaction or minor disturbance hinted at with a small, diffuse extension. The galaxy's overall color suggests it is a relatively massive system.
