The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing nearly circular in projection. The light distribution shows a strong central bulge, diminishing gradually outwards. Color gradients are subtle, with a possible tendency towards redder hues in the core region. There appears to be minimal evidence of spiral arms or significant dust lanes. Overall, it is categorized as a quite regular-shaped galaxy. Indications suggest little to no ongoing major merger activity or strong tidal disturbances are present.
