The galaxy appears to be a relatively small, elongated system with a smooth, concentrated central bulge. The disk component is faintly visible and seems to be oriented edge-on or at a high inclination relative to our line of sight. There is some color variation across the galaxy; the central bulge exhibits a yellowish or reddish hue, while the disk appears slightly bluer. This suggests older stellar populations in the bulge and ongoing or recent star formation within the disk. The overall structure of the galaxy is relatively undisturbed, showing no signs of major mergers or significant tidal interactions. Based on its morphology, it can be described as a relatively undisturbed disk galaxy.
