The galaxy presents as a largely featureless elliptical morphology. It exhibits a concentrated, bright central region which gradually diffuses outwards. The color profile suggests an older stellar population, trending towards redder wavelengths, although some bluer light is still observed. The galaxy appears to be largely undisturbed, with no apparent tidal features or signs of a major merger event. It shows a high degree of central concentration. The overall impression is of a relatively massive and evolved galaxy.
