The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a moderate ellipticity, appearing somewhat more rounded than elongated. The color profile suggests an older stellar population, with a yellowish-red hue dominating the light emitted. There is no obvious spiral structure, bar, or prominent dust lanes visible. The object appears largely undisturbed, with no major signs of ongoing mergers or tidal interactions. A fainter, similarly colored object is also visible. Although not obviously interacting, its proximity suggests it may be a companion galaxy. Based on its general characteristics, it may be classified as an elliptical galaxy with evidence for a neighboring galaxy.
