The galaxy appears to be a spiral galaxy viewed at an oblique angle, revealing some disk-like structure. It displays a prominent central bulge, which seems to dominate the overall light profile. The bulge exhibits a smooth, featureless appearance. Traces of spiral arms are faintly visible, but they are not well-defined or tightly wound. The galaxy's color is generally yellowish-white, indicating an older stellar population with relatively low star formation activity. There is no significant evidence of dust lanes or strong star-forming regions, which supports the idea that the galaxy is not undergoing intense star formation. The galaxy does not show signs of recent major mergers.
