The galaxy presents as a system with intermediate morphology, displaying characteristics of both elliptical and spiral galaxies, but closer to an elliptical morphology. There is a high degree of central concentration, indicated by the bright, yellowish core, suggesting an older stellar population dominating the center. The overall shape is somewhat elliptical with a high degree of 'in-between' roundness and a low percentage of being cigar shaped, transitioning to a fainter, more diffuse halo. Faint blue regions, possibly indicative of star formation, are present in the outer regions, but they are not well-defined spiral arms. There are some apparent irregularities but no evidence of major mergers. There appears to be a minor disturbance present, which could be signs of a minor merger. The galaxy demonstrates a smooth structure with no clear dust lanes.
