The galaxy presents as an elongated, disk-shaped structure, observed nearly edge-on from our vantage point. It exhibits a pronounced central bulge that appears relatively smooth and featureless, indicating a high concentration of older stellar populations. The disk component is visible as a thin, faint band extending outwards from the central bulge. Evidence suggests the presence of some level of dust obscuration within the disk, particularly closer to the mid-plane. There is no clear presence of spiral arm structure. The overall color profile of the galaxy indicates a relatively red stellar population throughout the observed structure, suggesting low ongoing star formation. There are no indications of any major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears to be a relatively undisturbed disk galaxy observed at a considerable cosmological distance.