The galaxy presents a generally smooth and elliptical morphology, appearing predominantly spheroidal in shape. There is little evidence of distinct spiral arms or significant dust lanes. The central bulge is relatively prominent and concentrated, exhibiting a bright, yellowish hue suggesting an older stellar population. Moving outwards from the core, the light appears to fade and transition to a more diffuse halo with subtle blueish tints. The galaxy's overall form tends to be more rounded than elongated, and there are slight asymmetries in the outer regions, suggesting possible minor gravitational interactions or tidal disturbances. There are no signs of ongoing major merger activity, although low-level disturbances cannot be ruled out.
