The galaxy presents as a flattened elliptical or lenticular structure with a distinct central bulge. The luminosity appears to be relatively concentrated towards the core, gradually fading towards the outer regions. The overall color is predominantly reddish-yellow, with a slight hint of green towards the edges, suggesting the presence of an older stellar population. The galaxy displays a high degree of smoothness and symmetry, with no apparent spiral arm structures or significant irregularities. The morphological classification indicates it is primarily a smooth galaxy with a low probability of recent or ongoing merger activity. The galaxy has an apparent axis ratio of approximately 0.5 and a relatively small angular size, and has a significant sersic index which means it is not following a gaussian profile, but may instead be following a power-law trend.