The galaxy presents a generally smooth, rounded morphology. The central region is significantly brighter and exhibits a distinct greenish-blue hue, possibly indicating active star formation or the presence of an active galactic nucleus. The outer regions appear less concentrated and display a more diffuse, reddish-orange color gradient. This color variation suggests differing stellar populations, with older, redder stars dominating the outer regions. There is some indication of minor irregularities or disturbances in the galaxy's structure, though these are not particularly pronounced. There may be a merger occurring. The overall shape appears close to round.
