The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution is centrally concentrated, with a noticeable radial decrease in surface brightness moving outwards from the core. The central region displays a yellow-white hue, suggestive of an older stellar population, whereas the outer regions exhibit a slightly bluer tint, hinting at the presence of some younger stars, but not prominently. The overall form is neither perfectly circular nor highly elongated, appearing somewhere in between. There is no obvious sign of spiral arms, rings, bars, or prominent dust lanes. The galaxy appears largely undisturbed; no tidal tails, shells, or other signatures of recent major mergers are immediately apparent. Overall, it exhibits characteristics consistent with a spheroidal galaxy undergoing relatively low levels of star formation.
