The galaxy presents an elliptical morphology, exhibiting a smooth, featureless structure indicative of an evolved system. The central bulge appears prominent and concentrated, displaying a yellowish-orange hue suggesting an older stellar population. The disk component, while present, is less pronounced, showing a subtle flattening. A faint, bluish tinge is observed at the extremities of the galaxy, possibly indicative of ongoing, albeit limited, star formation. The galaxy's overall color gradient suggests a radial variation in stellar populations, with older stars concentrated towards the center and younger stars more sparsely distributed in the outer regions. There are some signs of minor disturbances in its shape. The general appearance is that of a somewhat massive galaxy.
