This galaxy presents a largely smooth morphology. The light distribution appears centrally concentrated with a somewhat circular isophote shape, though some minor deviations are present. There is some indication of a faint, diffuse halo or envelope extending beyond the main body of the galaxy. The color gradient suggests a higher concentration of older stellar populations towards the center, exhibiting redder hues, and slightly bluer colors in the outer regions, indicating more recent or ongoing star formation, though at an overall low rate. There is also a possible disturbance on the left side of the galaxy, indicating a possible past interaction with another object.
