The galaxy presents as a somewhat elongated, cigar-shaped object. A prominent central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population and potentially lower star formation activity in this region. The surrounding disk appears relatively smooth, with a faint bluish tint at the edges. The overall color gradient indicates a possible transition from an older stellar population in the bulge to younger, hotter stars in the outer regions of the disk. There is no clear evidence of strong spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of a major merger event. Overall it shows traits of a spiral galaxy, although the structure is not well-defined.
