The galaxy presents as a relatively smooth, elliptical object. The core exhibits a concentrated, bright intensity, with a discernible red-orange hue, suggesting a population of older stars. The isophotes appear generally elliptical with no obvious signs of a strong bar or spiral structure. A faint blue-ish halo surrounds the central bulge, indicative of a younger stellar population, or potentially some ongoing star formation activity although it appears minimal overall. There are some suggestions of tidal disturbances or a possible ongoing minor merger; with some faint asymmetries and non-smoothness in the outer regions, it is also possible that it is simply a merger remnant in its final stages of relaxation. Overall the galaxy is largely undisturbed.
