The galaxy presents as a largely featureless, elliptical-like structure. The core exhibits a concentrated, bright yellow hue, suggesting an older stellar population dominating the central region. The light profile appears smooth and radially decreasing from the center, with no discernible spiral arms or distinct dust lanes. The overall morphology indicates a highly spheroidal shape. There are no apparent signs of recent major merger activity or significant tidal disturbances. Its smooth appearance suggests that any merging events were likely in the distant past.
