This galaxy appears to be an elongated, cigar-shaped system. Its light is concentrated towards the center, with a gradual decrease in brightness as you move outwards towards its edges. The color gradient transitions from a slightly bluer hue in the central region, to a redder tint toward the extremities. This color shift suggests a varying stellar population within the galaxy, with perhaps younger, hotter stars concentrated in the core and older, cooler stars populating the outer regions. No distinct spiral arm structures are visible, suggesting a more spheroid or elliptical morphology. There may be a slight asymmetry in the overall structure of the galaxy, but no clear signs of major disturbances or ongoing merger events are evident in the image. 
