The galaxy presents as an elliptical or lenticular morphology, exhibiting a predominantly smooth light distribution. The object displays a moderate ellipticity, appearing as somewhat elongated rather than perfectly spherical. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy's central bulge region is bright, suggesting a concentration of older stellar populations. There is very little evidence of active star formation, indicated by the relatively homogenous color distribution across the galaxy's extent. Any discernible features are subtle, potentially indicating minor tidal interactions or disturbances in the galaxy's outer regions, but these are minimal. Overall, the galaxy appears relatively undisturbed and evolved, consistent with a redder, quiescent system.