The galaxy exhibits an overall elliptical morphology, appearing significantly elongated. A central bulge is visible, displaying a concentrated luminosity gradient transitioning outwards to a fainter, more diffuse halo. The light distribution appears relatively smooth with no prominent spiral arm structures or significant dust lanes discernible. Color gradients suggest a population of older stars dominates, with a bluer hue in the outer regions. It is a galaxy of intermediate size and stellar mass.
