The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outwards. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the galaxy's light output. There are no discernible spiral arm structures or significant dust lanes visible within the galaxy. Minor disturbances are possibly present based on some slight asymmetry and the lack of a perfectly spherical appearance but no major merger events are apparent. It displays a fairly round shape, appearing neither highly flattened nor elongated. Overall, this galaxy appears to be a quiescent, evolved system with minimal current star formation.
