The galaxy presents as a smooth, elliptical-like structure with a high degree of central concentration. Its color profile suggests a relatively evolved stellar population, exhibiting a yellowish-orange hue centrally, with fainter blue edges. The galaxy displays an elongated, cigar-like morphology. There is no obvious evidence of spiral arms or significant dust lanes. The overall structure appears undisturbed, with no indications of a recent major merger event, although there is the possibility of a minor disturbance. Its small angular size suggests a substantial distance.
