This galaxy presents as a flattened, disk-shaped structure, viewed nearly edge-on. A central bulge is visible, exhibiting a brighter, more concentrated luminosity, suggestive of an older stellar population. Fainter regions extend outwards from the bulge in a relatively smooth disk, with a blue tinge indicating more recent star formation within the galaxy. The disk appears to be slightly warped, with a faint, somewhat irregular distribution of starlight. There is no readily apparent dust lane bisecting the galaxy. It shows minimal signs of a recent or ongoing major merger event.
