The galaxy presents a largely smooth morphology. The light distribution is centrally concentrated, exhibiting a significant bulge component that graduates into an extended, fainter halo. The ellipticity appears moderate; the galaxy is neither perfectly circular nor highly elongated. 

There is a slight color gradient visible, with the central region appearing redder, possibly indicating a concentration of older stellar populations or dust obscuration in that area. The outer regions seem slightly bluer, potentially suggesting ongoing star formation, although the extent of this activity seems relatively low. There is no obvious presence of spiral arms or a prominent disk structure. No strong tidal features or signs of recent major mergers are apparent. However, very minor disturbances cannot be ruled out at this resolution.
