The galaxy presents as a spiral galaxy with a noticeable central bulge. The bulge exhibits a yellowish-white hue, potentially indicative of an older stellar population. Two prominent spiral arms emanate from the central bulge, extending outwards. These arms appear somewhat tightly wound and are bluer in color than the bulge, suggesting ongoing star formation regions within the spiral arms. The overall orientation of the galaxy appears to be slightly inclined to our line of sight, though not completely edge-on. The disk appears relatively smooth, with some evidence of dust lanes, likely obscuring star formation in some regions. There is a subtle hint of a bar-like structure bisecting the central bulge. The morphological features suggest a galaxy that has not experienced any major mergers recently, though the outer regions might be slightly disturbed, indicating some past interaction.
