The galaxy presents a generally smooth morphology. It exhibits a central bulge that appears relatively bright and concentrated, surrounded by a fainter, more diffuse halo or disk component. The overall shape is elliptical, verging on slightly elongated but not obviously cigar shaped. There is no clear evidence of spiral arm structure, and it does not appear to be undergoing a major merger, although some minor disturbances cannot be ruled out. Color gradients suggest a population of older stars dominating the galaxy, and it is likely a massive galaxy with a relatively low star formation rate.
