The galaxy presents as a relatively smooth, elongated structure. The primary body exhibits a concentrated central bulge, with a gradual fading outward into what appears to be a disk. There is a slight blue tint to the ends of the disk, but mostly the disk consists of a yellowish-white hue. The smooth appearance suggests a lack of significant ongoing mergers or major disturbances. The disk displays a noticeable lack of defined spiral arms or intricate dust lane structures. The central bulge displays the brightest and most prominent features of the galaxy, suggesting an older stellar population or a significant amount of dust obscuring the core. There is no strong evidence of active galactic nucleus activity visible in this image. Overall, the galaxy appears to be a disk galaxy with an intermediate inclination.
