The galaxy presents as a relatively smooth, elliptical-like structure. Its color suggests an older stellar population, leaning towards a reddish-yellow hue. There is no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy appears largely undisturbed, with no major signs of ongoing merger activity or tidal interactions with neighboring galaxies. The light distribution is centrally concentrated, indicating a possible bulge component. Overall, this galaxy appears as a fairly evolved system.
