The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge that dominates its overall light distribution. There is a noticeable radial gradient in surface brightness, with the core being significantly brighter than the outer regions. The galaxy displays a slight yellow-red hue, suggesting an older stellar population with relatively low levels of on-going star formation. No prominent spiral arms, dust lanes, or other distinct features are immediately visible. The shape appears close to circular on the plane of the sky, with minimal ellipticity observed.
