The galaxy presents as an elongated, disk-like structure, viewed at a high inclination relative to our line of sight. A central bulge region appears moderately concentrated and luminous, suggesting a stellar population that is, on average, older than the surrounding disk. The disk exhibits a mottled appearance, with slight variations in color, indicating possible regions of varying stellar density and star formation. The blueish tint along the disk hints at the presence of younger, hotter stars and ongoing star formation, especially at the edges. There is a subtle dust lane hinted on the galaxy, where the color is altered. The overall structure appears relatively undisturbed with no major mergers, though there may be some minor asymmetries or irregularities within the disk indicating some gravitational interaction. The galaxy displays a flattened ellipsoidal shape.
