The galaxy presents a roughly elliptical morphology, elongated along one axis. The core exhibits a high surface brightness with a yellow-white hue, suggesting a concentration of older stellar populations. This central region smoothly transitions into a less luminous, more diffuse halo. The halo displays a slightly bluer color than the core, hinting at the presence of younger stars or ongoing star formation in these outer regions. There is no clear evidence of spiral arm structure or a distinct dust lane. The overall appearance indicates a galaxy that may be relatively evolved, with a significant fraction of its stellar mass residing in the spheroidal component. There are some indications of minor tidal disturbances but no major mergers.
