The galaxy presents as a fairly smooth, centrally concentrated system. It exhibits a generally elliptical morphology, appearing nearly round. The central bulge is prominent, displaying a yellowish hue suggesting an older stellar population and relatively low levels of ongoing star formation. There is little evidence of spiral arm structure or significant dust lanes. The outer regions of the galaxy fade gradually into the background sky, indicating a lack of sharp edges or tidal features. Overall, the galaxy appears relatively undisturbed and does not show signs of any recent major merger events or strong gravitational interactions.
