The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a central concentration of light, indicative of a bulge component. There is a subtle elongation, deviating from a perfectly circular shape, suggesting a possible mild distortion. The color appears yellowish-orange, consistent with a stellar population dominated by older, redder stars. The overall structure lacks prominent features such as spiral arms or dust lanes. There is a possibility of it experiencing a minor gravitational interaction with a companion galaxy.
