The galaxy presents a primarily smooth morphology, with a likely disk structure viewed at an oblique angle. The central region exhibits a concentrated, bright core. There is a subtle color gradient extending outward from the core, transitioning from yellowish-orange to a greenish hue in the outer regions of the disk. This color variation suggests differential stellar populations and/or dust content. The galaxy’s shape is elongated, appearing somewhat cigar-shaped. There is no obvious presence of strong tidal features or morphological disturbances indicative of recent major merger events.
