The galaxy presents as an elongated, cigar-shaped object. It exhibits a smooth, relatively featureless morphology across its visible extent. A central bulge is visible, appearing brighter and more concentrated than the surrounding galactic disk. The galaxy's color gradient suggests a higher concentration of older stellar populations in the central regions, transitioning to slightly bluer hues in the outer regions. There is no evidence of spiral arm structure, significant dust lanes, or ongoing major mergers. The slight asymmetry in the outskirts might indicate minor gravitational interaction.
