The observed galaxy appears as an edge-on spiral galaxy, exhibiting a pronounced central bulge. The bulge displays a smooth, concentrated distribution of light, with a color gradient suggesting an older stellar population dominating its composition. A faint, extended disk is visible, bisecting the bulge and extending outwards. The disk appears relatively thin and uniform in its structure. There are indications of possible dust lane structures within the disk, obscuring some of the light emitted from behind. A small patch of redder light is seen within the disk, which may signify ongoing star formation. The overall morphology indicates a likely high inclination angle relative to our line of sight.
