The galaxy presents as a relatively smooth, elliptical or lenticular-like structure. It appears to be moderately bright and concentrated, with a luminous central bulge that graduates to a more diffuse outer region. The galaxy exhibits a subtle color gradient, transitioning from a yellowish-white core to a slightly bluer hue in the surrounding halo, potentially suggesting ongoing, but subdued, star formation in the outer regions. There is a very minor suggestion of distortion present, possibly indicative of past or ongoing interactions.
