This galaxy presents as a luminous, centrally concentrated object, potentially an elliptical or lenticular galaxy given its smooth appearance. The dominant color is a yellow-orange hue, suggesting an older stellar population. Its morphology is primarily smooth, with the majority of its light concentrated within a radius of approximately 8 kpc. There is a faint suggestion of minor disturbance or interaction occurring, possibly due to gravitational influence from a smaller companion. Although the galaxy's profile appears more elliptical than circular, the apparent roundness might be influenced by the viewing angle. Overall, this galaxy likely represents a relatively massive system with a quenched star formation rate, indicative of a more evolved stellar population.
