The galaxy presents a generally smooth, elliptical morphology with a dominant central bulge. The color gradient suggests a concentration of older stellar populations in the core, exhibiting a yellowish-orange hue. There is a subtle asymmetry in the light distribution, possibly indicating a minor interaction or internal disturbance. One side of the galaxy shows slightly elongated feature, like a faint tidal tail or an arm which could suggest a possible merger or interaction with another galaxy. Overall, the galaxy appears to be a relatively massive system with suppressed star formation and it appears round.
