The galaxy presents as a spiral type, exhibiting a relatively flattened disk structure. A central bulge is moderately apparent, appearing neither overly dominant nor negligible in size. Spiral arms are clearly discernible, wound rather tightly around the galactic center. The arms show some degree of fragmentation, hinting at active star formation regions within. No major disturbances or signs of a significant merger event are apparent, although subtle irregularities might be indicative of minor gravitational interactions. A faint bar is possibly present. The disk of the galaxy is positioned at a wide angle with respect to our line of sight.
