The galaxy presents as a flattened, disk-shaped structure, indicative of a spiral or lenticular morphology. It is observed nearly edge-on from our vantage point, obscuring detailed spiral arm features if present. A central bulge is visible, displaying a yellowish hue, suggesting an older stellar population dominating the core. The disk exhibits a bluer tint compared to the central bulge, implying the presence of ongoing or recent star formation in the outer regions. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or significant tidal interactions. The smooth appearance of the disk suggests a settled morphology with little to no significant asymmetric features.
