The galaxy presents a generally smooth, elliptical morphology, showing a concentrated central bulge. There is some evidence of a flattened disk-like structure extending from the central bulge. Color gradients suggest a central concentration of older, redder stellar populations, with a slightly bluer hue in the outer regions of the galaxy. No significant spiral arm structure or prominent dust lanes are visible. There are no signs of a recent major merger, although subtle tidal features and minor disturbances in the galaxy's outer regions cannot be ruled out.
