The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. It exhibits a spheroidal morphology with a high degree of central light concentration. The galaxy's overall color is yellowish-orange, suggesting a relatively old stellar population, where the more massive, blue stars have already evolved off the main sequence. There appears to be minimal evidence of spiral arms or significant dust lanes. Some faint, extended light is observed surrounding the main body of the galaxy, suggesting a halo of older stars or a diffuse stellar population. Any signs of recent star formation, such as bright blue regions, are conspicuously absent, further supporting the conclusion of an evolved stellar population. Based on its color and structure, it is likely the galaxy has little active star formation at present.
