This galaxy appears to be a spiral galaxy, viewed edge-on from our perspective. A prominent, elongated central bulge dominates the structure, displaying a smooth and concentrated brightness profile. The bulge color indicates an older stellar population. Fainter and more diffuse light extends from the central bulge, suggesting a relatively thin disk component. The disk appears tightly wound and relatively smooth. There is no visible evidence of active star formation regions, grand design spiral arms, or prominent dust lanes within the disk, suggesting a quiescent or slowly evolving system. The bulge appears more rounded than boxy, implying a possible lack of bar structure. There are no clear signs of tidal disturbances or ongoing mergers.
