The galaxy presents as a faint, somewhat irregular structure with a subtle disk-like morphology. The central region appears more concentrated with bluer hues suggestive of recent or ongoing star formation activity. The outer regions are less defined, fading gradually into the background sky. There are hints of tidal features, potentially indicating past interactions or mergers. These appear as faint extensions emanating from the main body of the galaxy, particularly to one side. The disk itself seems slightly warped or disturbed, which may support the merger or interaction hypothesis. Overall, the galaxy appears to be in a dynamic state.
