The galaxy presents as a flattened, elliptical shape, suggesting a possible disk galaxy viewed at an oblique angle. A prominent central bulge is visible, exhibiting a yellowish-orange hue, indicative of an older stellar population. The outer regions display a bluer tint, potentially indicating younger stars and ongoing star formation. The disk appears relatively smooth, with no distinct spiral arm structures immediately apparent at this resolution, though some subtle features may be present. There may be slight morphological disturbances present, but there is no major merger or significant interaction occurring.
