The galaxy presents as an edge-on spiral, with a notably prominent bulge. The bulge exhibits a smooth, centrally concentrated morphology, characterized by a rounded appearance. The disk is thin and elongated, oriented nearly perpendicular to our line of sight. No distinct spiral arm structure is discernible. There may be a faint, diffuse halo surrounding the main body of the galaxy, though this is uncertain given the image quality. There is no apparent ongoing major merger activity or strong tidal disturbances. The color gradient suggests a relatively older stellar population within the bulge.