The galaxy presents as a cigar-shaped system, with a smooth, centrally concentrated light profile. Its appearance suggests it is viewed nearly edge-on, leading to the elongated morphology. The central region displays a bright, concentrated luminosity. This implies a higher density of stars within the core.  Fainter and bluer diffuse light extends along the major axis, potentially indicating the presence of a stellar disk. No distinct spiral arms are discernible, nor is there evidence of prominent dust lanes, or strong star forming regions. There is no evidence of any major or minor mergers and no obvious tidal features. 
