The galaxy presents as a centrally concentrated, smooth system with a noticeable elliptical morphology. The core exhibits a bright, yellowish-white color, suggesting a significant population of older stars. The light profile appears to diminish gradually from the core outwards, with no obvious spiral arm structures or prominent dust lanes visible. 

A faint, diffuse halo surrounds the central region. The halo appears relatively homogenous in color, also suggestive of an older stellar population. There is only the slightest hint of blue, potentially very faint and small regions of active star formation. There are no obvious signs of major tidal disturbances or ongoing mergers, although some minor asymmetry in the outer isophotes cannot be ruled out. Overall, the galaxy appears to be relatively quiescent and evolved.
