The galaxy presents a clear edge-on disk morphology. A central bulge is visible, appearing moderately prominent and somewhat elongated. The bulge exhibits a rounded structure, lacking a distinct boxy shape. The disk appears relatively smooth, with a lack of apparent substructure such as spiral arms or dust lanes. The color distribution suggests a moderate degree of stellar population variation, with a redder central bulge possibly indicating an older stellar population, and slightly bluer hues towards the outer disk indicative of younger star formation. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The overall structure appears undisturbed and relatively quiescent.
