The galaxy presents as an elongated, somewhat cigar-shaped structure. It exhibits a central bulge region that appears yellowish, suggesting an older stellar population. Extending outward from the bulge, a faint disk is visible, with a bluer hue towards the edges implying more recent star formation activity. The galaxy appears relatively smooth, with only subtle indications of features such as spiral arms or dust lanes. There may be a hint of a minor disturbance in the morphology, suggesting a possible past interaction or merger event, but it is not a particularly prominent feature. The overall color of the galaxy indicates a transition between a predominantly old stellar population in the bulge and a younger one in the disk, suggesting ongoing, but moderate, star formation.
