The galaxy presents as a spiral type, observed at a slight angle, not quite edge-on. Distinct spiral arms are apparent, though somewhat diffuse. The color suggests active star formation regions, most pronounced within the spiral arms. A central bulge is discernible, appearing neither overly dominant nor negligible in size. The galaxy displays no obvious signs of major merger activity, although the structure of the spiral arms suggests some past gravitational interaction or minor disturbance. The presence of a bar structure is difficult to definitively determine, possibly a weak bar. Dust lanes are present within the spiral arms, contributing to their mottled appearance. The galaxy is relatively faint, indicating that it's either at a considerable distance or not a particularly luminous galaxy.
