This galaxy presents as a centrally concentrated object with a moderately smooth, but not entirely featureless, morphology. The central region exhibits a bright, concentrated core. Surrounding the core, a more diffuse, extended halo or disk-like structure is observed. The galaxy appears largely symmetrical and rounded in shape, with only subtle deviations from perfect circularity. There are some faint hints of disturbed structure, such as possible tidal tails, or minor asymmetries, suggesting potential interactions or past mergers, but nothing major. Its color index suggests a relatively high rate of star formation.
