This galaxy presents a mostly smooth, elliptical morphology. The central bulge exhibits a concentrated, yellowish-white luminosity suggesting an older stellar population. Surrounding the core, a bluer, more diffuse halo extends outwards, indicating the presence of some younger stars and/or a population with lower metallicity. The disk is subtle and not strongly defined, but is oriented at a slight angle to our line of sight. There appears to be very little active star formation currently occurring, although the outer regions do show hints of blue. The overall structure appears relatively undisturbed, with no obvious signs of a recent major merger event.
