The galaxy presents as a spiral, viewed at an oblique angle but not quite edge-on. A prominent bulge dominates the central region, exhibiting a yellowish-orange hue, likely indicating an older stellar population. The disk shows evidence of spiral arm structure, though the arms are not sharply defined. The winding of the arms appear moderately wound. The bluer color observed in the outer regions of the disk suggests the presence of younger, hotter stars and ongoing star formation. There is evidence of a bar structure, with a faint bar visible across the central bulge region. There is a visible distortion in the morphology, indicating possible interactions with other galaxies. 