This galaxy appears to be a relatively smooth, centrally concentrated system, likely an elliptical or lenticular galaxy. Its shape is elongated, with an apparent axis ratio suggesting it's seen at an intermediate angle rather than face-on. There is a slight color gradient, with the central bulge exhibiting a yellowish-orange hue, possibly indicating an older stellar population. Fainter, bluer light appears more prominent in the outer regions, which may imply some ongoing or recent star formation, although it is not obvious. Based on the lack of prominent spiral arms or significant dust lanes, the galaxy appears to be relatively evolved. There is no obvious evidence of any major merger activity or tidal disturbances affecting its overall morphology. The galaxy appears to be a fairly isolated system.
