This galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The color gradient suggests a more aged stellar population dominating the galaxy's light output, particularly in the central regions which appear yellowish. There is a subtle decrease in brightness moving outwards from the core with a slight redder tinge. It seems to exhibit high degree of roundness in its overall shape. There is little to no evidence of spiral arms, bars, or significant dust lanes. The overall structure suggests a system that has undergone significant morphological evolution, likely with little ongoing star formation.
