The galaxy presents as a centrally concentrated structure with a largely smooth morphology. The overall color is yellowish-white, suggesting a dominant population of older stars, although the central region appears somewhat brighter and possibly bluer, which could indicate a region of ongoing, albeit mild, star formation. The isophotes are moderately elongated, but the galaxy does not exhibit a clear spiral arm structure or other distinct features typically associated with disk galaxies. There are hints of slight disturbances or asymmetries in the outer regions, possibly indicative of a past minor merger event, however, the image resolution makes definitive confirmation difficult.
