The galaxy presents a generally smooth and elliptical morphology. It appears nearly spheroidal, exhibiting a high degree of central concentration with a gradually decreasing luminosity profile toward its outer regions. The color gradient suggests a redder, likely older stellar population dominating the galaxy's core. The outer regions show a hint of bluer hues, possibly indicating pockets of more recent star formation, though at a low rate. There is no clear evidence of spiral arms or a distinct disk structure. The overall appearance is consistent with an early-type galaxy with no significant signs of ongoing mergers or major tidal disturbances.
