The galaxy presents as a roughly elliptical shape, exhibiting a disk-like structure viewed at a moderate inclination. The central region is significantly brighter and more condensed than the outer regions, suggesting a concentration of older stars or the presence of an active galactic nucleus, though this cannot be definitively confirmed from this image alone. The outer disk appears relatively smooth. There is evidence of an internal feature within the central bulge. This could be a dust lane obscuring part of the central structure, or a small, distinct nucleus. There are no obvious spiral arms or other major structural features visible in this image. The overall color suggests a moderate redshift, typical of distant galaxies. No strong evidence of ongoing major merging activity is present.
