The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a slight elongation. A bright, yellowish core dominates the central region, indicating a high concentration of stars, possibly an aging stellar population. Fainter, bluish light extends outwards from the core, suggesting the presence of younger stars or ongoing star formation. There are no apparent spiral arm structures or distinct dust lanes visible in the image. The galaxy exhibits a minor disturbance or irregularity in the outer regions, possibly a sign of a past minor merger event.
