The galaxy presents as a relatively faint, disk-shaped structure, oriented edge-on. The central bulge exhibits a smooth, concentrated light profile with a yellowish hue, suggesting a population of older stars. A dust lane, although not sharply defined, appears to bisect the galaxy along its major axis, absorbing some of the light from the stars behind it. The disk itself is thin and elongated, extending outwards from the bulge. The outer regions of the disk appear bluer in color, indicating the presence of a younger stellar population and potentially ongoing star formation. The overall morphology is suggestive of a late-type spiral galaxy, seen at a high inclination angle. There are no obvious signs of major mergers or significant tidal disturbances.
