The galaxy presents as a cigar-shaped, elongated object, likely a highly inclined or edge-on spiral or lenticular galaxy. It exhibits a smooth, diffuse light profile across the central region, suggesting a relatively uniform stellar population distribution or a prominent bulge component. There is evidence of a slightly bluer color component along the edges, potentially indicative of younger stars or active star formation regions within a disk structure. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. The overall morphology suggests a galaxy that is relatively settled and undisturbed.
