The galaxy presents as a somewhat elliptical structure, with a centrally concentrated bulge of primarily yellow-orange hues, suggesting an older stellar population. There is little evidence of spiral arms or distinct features, giving it a relatively smooth appearance. The galaxy appears quite round. The outer regions fade into a diffuse halo, appearing less concentrated than the central bulge. There is a subtle hint of blue tint on the far left of the halo, possibly indicating some recent star formation. No significant dust lanes or prominent star-forming regions are visible. The galaxy does not obviously appear to be undergoing a major merger event.