The galaxy presents as an elliptical morphology, appearing largely smooth with minimal discernible substructure within its light profile. The primary color is a yellow-orange hue, suggesting a stellar population dominated by older, redder stars and indicative of lower star formation activity. Its relatively high degree of roundness suggests it is closer to an E0 or E1 classification on the Hubble sequence. There is some subtle irregularity in the outer isophotes of the galaxy, possibly suggesting a minor interaction with a smaller companion galaxy or tidal disturbances. 
