The observed galaxy appears to be a spiral galaxy, characterized by a prominent central bulge. The bulge exhibits a smooth, concentrated light distribution, transitioning into a disk-like structure. Within this disk, spiral arms are visible, though somewhat flocculent and not sharply defined. The arms are traced by regions of brighter, blue-ish light, suggestive of ongoing star formation activity. There may be the presence of a weak bar structure within the central region. The overall color of the galaxy is relatively blue, indicating a population of young, hot stars. It is also plausible to interpret the presence of a merger or tidal disturbance in the faintness of the arms.
