The galaxy appears to be a spiral galaxy, presenting a near edge-on perspective. There is a central bulge that has a smooth appearance, likely consisting of older stellar populations. The disk exhibits some texture, potentially indicating the presence of spiral arms. The galaxy displays a color gradient, appearing bluer in the outer regions and redder towards the central bulge, suggesting ongoing star formation in the disk and a relatively older population in the bulge. The overall structure indicates that it could be in a relatively stable state, without significant signs of major mergers or tidal disturbances. Some minor irregularities are visible, but could be due to smaller interactions, star formation or dust. The galaxy is relatively small, and is likely to be a lower mass spiral galaxy.
