The galaxy presents as a cigar-shaped morphology, displaying a relatively smooth profile. There is a distinct color gradient noticeable, transitioning from a yellowish-white core region to bluish-white outer regions, suggesting ongoing star formation. The central bulge appears prominent and centrally concentrated, while the outer regions show a hint of a disk-like structure, but it is not well-defined. There is no evidence of strong spiral arms or significant dust lanes. Overall, the galaxy exhibits a regular structure with no signs of major disturbances or merging activity.
