The galaxy presents as a roughly elliptical structure, exhibiting a smooth overall morphology. The central region is dominated by a concentrated bulge that is bright and appears yellowish in color, suggesting a population of older stars. Moving outward from the center, the galaxy smoothly transitions to a fainter, less defined halo. The overall color gradient indicates a potentially diminishing stellar population density with increasing radius. There is a subtle hint of a disk-like structure, though the smoothness indicates the absence of prominent spiral arms. No significant dust lanes or areas of intense star formation are immediately apparent. There are also no signs of active galactic nuclei or galaxy mergers.
