The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. There is little discernible disk structure or pronounced spiral arm presence. The galaxy is mostly ellipsoidal in shape, appearing close to circular, with a slight deviation towards an intermediate form rather than an elongated or cigar-like structure. There are no apparent major mergers, or tidal disturbances, that severely disrupt its structure; the galaxy appears relatively isolated and relaxed. The object exhibits a yellowish hue in the optical bands, indicating a dominant population of older stars, this aligns with the galaxy being classified as relatively massive with a low rate of ongoing star formation. The galaxy has absolute magnitudes that indicate it is a relatively luminous object.
