The galaxy presents as a centrally concentrated, elliptical morphology with a smooth appearance. There is a distinct bulge that transitions into a more diffuse outer region. The galaxy's color profile suggests an older stellar population, with a yellowish-white hue in the central bulge region. The overall shape is slightly elongated but appears mostly rounded, not exhibiting a particularly strong disk component. There is no apparent evidence of spiral arms or significant dust lanes. No major disturbances or merging features are observed, though there are minor asymmetries. The galaxy appears relatively undisturbed.
