The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical or S0 type. There is little evidence of spiral arm structure or significant dust lanes. The central region of the galaxy exhibits a concentration of light, indicating a possible bulge component. The galaxy appears to be fairly isolated, without obvious signs of major tidal interactions or mergers. The overall color is relatively red, implying an older stellar population and suppressed star formation. There is a very slight hint of bluer light in the outer regions, but this is minimal. There might be minor disturbances, perhaps small satellite galaxies being accreted, or recent small merger events.