The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards, indicating a lack of prominent spiral arms or distinct features. The galaxy displays a yellowish-white hue in its core, suggesting an older stellar population. There's a slight elongation in its shape, with an axis ratio suggesting a flattened ellipsoidal form. Minimal signs of tidal disturbances or mergers are apparent from its overall structure, although there are hints of slight asymmetry in the outer regions. Based on the color and morphology, the galaxy is likely a massive system with a reduced star formation rate.
