This galaxy appears to be a spiral galaxy, observed nearly edge-on. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity indicative of a high stellar density. The disk appears relatively thin, with some evidence of dust lanes partially obscuring the light from stars within the galactic plane. The disk exhibits a noticeable blue hue, especially towards the outer regions, which is indicative of ongoing star formation. Faint spiral arms are suspected, though difficult to discern due to the edge-on perspective. The galaxy appears to have undergone some type of merger event in the past, given it's irregular shape.
