The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. Its core is notably brighter and appears yellowish, suggesting an older stellar population dominates the central region. Moving outward from the core, the galaxy's color shifts towards a slightly bluer hue, indicating the presence of some younger stars within the galaxy's extended halo. No distinct spiral arm structures are discernible. The galaxy shows no obvious signs of a major ongoing merger event, however there may be minor disturbances or tidal features, given the somewhat irregular edges of the galaxy. Overall, the system appears to be a relatively massive galaxy, likely past its peak star formation phase.
