The galaxy presents a smooth, elliptical morphology. It exhibits a central bulge with a high degree of symmetry, surrounded by a diffuse halo that gradually fades into the background. The galaxy's overall shape appears somewhat elongated, closer to an intermediate elliptical classification. There is minimal evidence of distinct spiral arm structures or dust lanes; however, it appears more blueish in color implying it could be in the process of forming more stars. There are no visible signs of ongoing major mergers or tidal disruptions, but there is a faint outer halo that gives off hints of minor disturbances or past interactions.
