The galaxy presents as a fairly smooth, elliptical-like structure with a bright, concentrated central bulge. The color appears generally yellowish, suggesting a population of older stars. There is a very faint, diffuse halo extending slightly beyond the main body of the galaxy. There is no apparent spiral arm structure. The overall appearance is consistent with an early-type galaxy that has largely exhausted its gas supply and has a low current star formation rate. There may be minor signs of tidal disturbance or interaction based on the faint asymmetry in the outer halo, but this requires further investigation. The galaxy does not appear to be undergoing a major merging event.