The galaxy presents as a largely homogenous, elliptical structure. It exhibits a high degree of central concentration, with a bright, yellowish core that fades into a reddish halo. The overall form is consistently smooth, lacking apparent spiral arms or distinct features typically associated with disk galaxies. There is minimal evidence of substructure or tidal disturbances, suggestive of a relaxed system potentially resulting from the end stages of galaxy evolution. The galaxy appears to be well-defined and is more rounded than cigar-shaped. There is no evidence of significant recent star formation, and it appears to have a low specific star formation rate. There is no evidence of a recent merger, although a minor disturbance cannot be ruled out.
