The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The color profile shifts gradually from a yellowish-white core to a reddish-orange halo, indicative of an older stellar population, concentrated towards the center, and a less aged population in the outer regions. The morphology is largely undisturbed, with no signs of ongoing major mergers or tidal features, although there are minor disturbances of sorts. There is a clear lack of distinct spiral arms or prominent dust lanes. The object appears largely spheroidal, with only a slight deviation from perfect circularity. The object has a median star formation rate that is quite slow, relative to the galaxy's mass.
