The galaxy presents an elliptical morphology, appearing as a diffuse, concentrated spheroid of light. Its color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue characteristic of lower star formation rates. The isophotes appear relatively smooth, with little indication of spiral arm structures or significant dust lanes. The shape exhibits a moderate ellipticity, leaning towards a more oblate form rather than perfectly spherical. There is no immediately apparent evidence of tidal disturbances or ongoing major mergers, although subtle asymmetries might be present upon closer inspection. Based on the overall appearance, this galaxy is likely a relatively quiescent system with minimal active star formation.
