This galaxy exhibits a distinct lenticular, or possibly spiral, morphology with a clear disk component. The disk is oriented edge-on from our line of sight. The central bulge appears prominent and has a yellowish hue, likely indicating an older stellar population. The outer disk regions appear fainter and exhibit a bluer color. This suggests ongoing star formation in the outer parts of the disk, in contrast to the older bulge. The galaxy displays a smooth appearance, with no immediately apparent signs of recent major mergers or tidal disturbances in its morphology. However, close inspection reveals minor irregularities and potential for some small-scale ongoing or past interactions.
