The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color profile indicates a dominant population of older stars, with a central concentration of yellow-orange light suggesting a bulge. The galaxy lacks prominent spiral arms or a clear disk-like structure. There is a subtle elongation along one axis, suggesting it is not perfectly spherical. Minimal, if any, dust lanes are visible, and there are no indications of active star-forming regions, based on a lack of blue hues and other indications of star formation. No signs of tidal disturbances or ongoing major merger events are readily apparent, but there might be minor disturbances.
