The galaxy presents a generally smooth, rounded appearance, suggesting an elliptical morphology or a disk galaxy seen face-on with minimal spiral structure. There is a central concentration of light which decreases smoothly in intensity outwards, exhibiting a diffuse halo. The light profile is consistent with a galaxy that is mostly bulge dominated. There may be a hint of faint blue light in the halo, but the object overall has a yellow-red hue. There is no apparent spiral structure, bar, or other prominent features usually associated with disk galaxies. The galaxy is not currently experiencing any major merging activity, but there may be minor disturbances in the galaxy's halo suggesting past interactions. The object is considered fairly large.
