The galaxy presents a largely smooth, elliptical morphology. It appears to be a relatively round object with no immediately obvious signs of spiral arms or a prominent disk. The galaxy exhibits a centrally concentrated brightness profile, with luminosity decreasing gradually outwards. It shows a yellowish color, suggesting an older stellar population with relatively low ongoing star formation, with potentially some dust obscuration. There appears to be no strong evidence of a major ongoing merger event or significant tidal disturbances. The overall structure indicates a gravitationally relaxed system.
