This appears to be a spiral galaxy seen nearly edge-on. The central bulge is prominent and elongated along the major axis, displaying a yellowish-white hue. The disk appears relatively thin, exhibiting a bluish tint, suggesting the presence of younger stars.

There are hints of dust lanes visible in the disk, particularly near the central bulge.

The overall structure suggests a system that may have experienced some gravitational interaction, either a minor merger or tidal disturbance, based on the slight asymmetry observed. The galaxy shows evidence of ongoing, but low, star formation activity.
