The galaxy presents as a yellowish, ellipsoidal structure. It appears mostly smooth, with a high degree of central concentration that fades outwards. The galaxy shows an elongated shape, being more "in-between" a disk shape or cigar shape. There is some indication of a slight warp or twist in the outer regions, though this could also be an artifact of the viewing angle or image processing. No clear spiral arm structures or prominent dust lanes are discernible. There is no evidence of a major ongoing merger. The overall color suggests a population of older stars, with a very faint blueish tint at the edges.
