The observed galaxy presents as a flattened, disk-like structure viewed nearly edge-on. A prominent central bulge is visible, appearing more concentrated and yellowish in color, suggesting an older stellar population. The disk itself appears elongated and somewhat diffuse, displaying a bluer hue towards the outer edges, possibly indicative of ongoing or recent star formation within the spiral arms or disk. Evidence of dust lanes is subtle but potentially present as darker, less distinct regions within the disk, close to the central bulge. The overall structure suggests a spiral galaxy with a prominent bulge.
