The object presents as a spiral galaxy, inclined at a significant angle relative to our line of sight. The central bulge is prominent and elongated, suggesting the presence of a bar structure within the galaxy. Faint spiral arms extend from the central region, displaying a somewhat flocculent morphology. The disk appears relatively smooth, with a noticeable absence of bright star-forming regions, indicating a potentially quiescent or slowly evolving system. The isophotes suggest a Sersic profile with a moderate concentration. Overall, the galaxy exhibits characteristics consistent with an intermediate-type spiral, possibly undergoing a period of suppressed star formation.
