The galaxy presents an elliptical morphology, appearing relatively smooth and featureless. Its light profile suggests a concentrated central bulge region, characterized by a yellowish-orange hue, indicative of an older stellar population. The galaxy exhibits a moderate degree of elongation, with its shape described as between round and cigar shaped. There is no obvious evidence of spiral arms or significant dust lanes within the visible spectrum. It shows no signs of a major merger but perhaps a minor disturbance may be present. Overall, the galaxy gives the impression of being a relatively undisturbed, evolved system with ongoing though fairly limited star formation.
