The observed galaxy presents a distinct, elongated morphology suggestive of a spiral galaxy viewed nearly edge-on. The galaxy exhibits a concentrated central bulge that appears relatively smooth. The disk component appears thin and extended, with a length significantly greater than its width. There is a slight asymmetry in the disk's brightness distribution, potentially indicative of a minor gravitational disturbance or interaction. The galaxy's color is generally yellowish, with some faint bluer regions visible, possibly corresponding to areas of recent star formation. No prominent dust lanes are readily apparent in this image, though this may be due to the viewing angle. Overall, the galaxy appears to be a moderately massive system with ongoing star formation.
