The galaxy presents a generally smooth and elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellow-orange in color, indicative of an older stellar population. The surrounding halo or disk component is faint and less structured, showing a gradual decrease in light intensity outwards from the core. There's a very slight elongation to the galaxy, suggesting it might not be perfectly spherical, tending towards a slightly flattened ellipsoid shape. No distinct spiral arms or dust lanes are visible; the overall appearance indicates a lack of significant ongoing star formation. The galaxy appears relatively isolated, showing no clear signs of tidal interactions or major disturbances in its structure. There are no apparent signs of a recent or ongoing merger event.