The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, which fades into a less-defined, more diffuse halo. The overall color is consistent with an older stellar population; hints of bluer hues can be observed but it presents as predominantly redder. No distinct spiral arm structures or significant dust lanes are apparent. The shape appears elongated, but not excessively so, falling between perfectly round and a highly elongated form. There is no obvious evidence of ongoing major mergers, though some minor tidal disturbance or interaction cannot be ruled out, based on slight irregularities in the outer halo.
