The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light profile. The major axis of the galaxy appears roughly three times its minor axis, indicating a cigar shape and moderately high ellipticity. The core region is a relatively bright yellowish hue and there is a slight bluing in the fainter outer edges of the galaxy. No distinct dust lanes, spiral arms, or other prominent features are readily apparent. The overall structure suggests minimal ongoing merger activity or significant internal disturbance. The lack of clear features indicative of active star formation areas implies a relatively quiescent or evolved stellar population.
