The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution. The central region is highly concentrated and luminous, with a yellow-white color suggestive of an older stellar population. The light profile diffuses outwards from the core, gradually decreasing in intensity. There is a subtle hint of bluer light in the outer regions, potentially indicating the presence of some younger stars, however it does not appear significant. The overall structure is relatively undisturbed, lacking any obvious signs of tidal tails, shells, or strong asymmetries, suggesting it is not undergoing a major merger event. The galaxy appears to be relatively isolated in its environment. 
