The galaxy presents a largely smooth, elliptical morphology. It appears somewhat rounded, though not perfectly spherical, with a slight elongation visible along its major axis. The central region exhibits a high degree of luminosity, indicative of a concentrated stellar population. The colour gradient shifts from a yellowish core to slightly redder hues in the outer regions. There is no clear evidence of prominent spiral arms or a distinct disk structure. Subtle irregularities may exist in the outer halo, suggestive of minor disturbances, although no major merging events are immediately apparent in the image.
