The galaxy appears to be a relatively compact object, approximately 6 arcseconds in diameter. The central region exhibits a high surface brightness, appearing almost uniformly bright and unresolved. There is a subtle color gradient within the galaxy, with a somewhat bluer core gradually transitioning to redder outer regions. The morphology suggests a centrally concentrated structure; it is quite smooth, showing minimal apparent spiral structure or distinct features. There are slight indications of minor disturbances in the outer edges of the galaxy, which could indicate tidal interactions. The light distribution surrounding the core seems relatively symmetrical, though it is not perfectly circular.
