This galaxy presents a largely smooth morphology, exhibiting a centrally concentrated light profile. The galaxy appears elliptical in shape, with an intermediate roundness classification, neither perfectly circular nor highly elongated. There is no obvious evidence of strong tidal features or major disturbances that would indicate a recent or ongoing major merger event, however, there are minor disturbances present. The core of the galaxy displays a yellowish-orange hue, possibly indicative of an older stellar population dominating this region. Fainter, bluer outskirts may suggest the presence of younger stars, but these are not very prominent.
