The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Color gradients suggest the presence of differing stellar populations and/or dust distribution. The core exhibits a distinct pinkish hue, potentially indicating a region of ionized gas or ongoing star formation, even if at a relatively low rate. The outer regions of the galaxy appear more diffuse with a greenish tinge. The overall morphology suggests a system that is unlikely to be undergoing any major merging events or significant tidal interactions. The observed roundness indicates it is viewed face-on.
