The galaxy appears as a centrally concentrated elliptical, exhibiting a smooth luminosity profile with a relatively high degree of central concentration. It presents an overall yellowish-white hue, indicative of a stellar population dominated by older, evolved stars. There is no obvious disk structure or spiral arm morphology visible; the light smoothly declines from the center outwards. There is no indication of ongoing active star formation. The object appears isolated and relatively undisturbed, with no signs of major tidal interactions or recent mergers. The galaxy has a somewhat round shape, not appearing too elongated or cigar-shaped. There might be very minor disturbances present, but they are difficult to notice.
