The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated bulge, suggesting a significant population of older stars. Moving outward from the core, the galaxy displays a relatively smooth structure. There is evidence of a surrounding disk component. The spiral arm structure is not prominent, and it appears smooth overall with little to no clumpy star formation. A distinct color gradient is observed, transitioning from a yellowish-orange hue in the center to a bluer tint in the outer regions, which might imply some active, yet subdued star formation. There is no indication of major disturbances or ongoing merging events.
