The galaxy presents as a relatively small, elongated object with a smooth, featureless appearance. It is likely a disk galaxy, viewed edge-on, with a cigar-like shape. The central region of the galaxy exhibits a slightly brighter, more concentrated luminosity, possibly indicating a central bulge or a higher density of stars and dust. A blueish tint is visible along the major axis, which could be associated with star formation. There is no evidence of a spiral structure or significant dust lanes, which further supports the edge-on orientation. No signs of major disturbances or ongoing merging events are visible.
