This galaxy appears to be a spiral galaxy, observed at a near edge-on inclination. The central bulge is prominent and displays a smooth, concentrated morphology, with a bright, almost uniform glow. This suggests an older stellar population dominates the bulge. Extending outwards from the bulge, we can see evidence of a faint galactic disk. The disk appears slightly warped, with the dust lanes along the edge on view. The disk appears to be blue, implying a somewhat active star formation rate. The overall structure appears relatively undisturbed, and the majority of citizen scientist labels it as not merging. I estimate the stellar mass is about 10^9.6 solar masses. It displays a low specific star formation rate. The apparent size is small, indicating that it is a very small or far away galaxy.
