The galaxy exhibits a largely smooth morphology with hints of disk-like structures. The galaxy appears somewhat rounded in shape. The central region displays a higher concentration of light and a yellowish color, potentially indicating an older stellar population. The outer regions of the galaxy are less concentrated, appearing fainter with a slightly bluer hue, possibly indicative of younger stars or ongoing star formation. No strong signs of major mergers or significant tidal disturbances are visible. Faint spiral structure or bar features may be present but are poorly defined. The overall appearance suggests a galaxy in the process of transitioning from a more actively star-forming phase to a quiescent phase.
