The galaxy presents a cigar-shaped, highly elongated morphology. The central region exhibits a yellowish hue, possibly indicating an older stellar population. This core appears relatively smooth and concentrated. Moving outward from the center, the color transitions towards a bluer shade, particularly at the extremities of the major axis. This suggests the presence of younger, hotter stars and regions of active star formation in the outer regions. While the galaxy does not show any significant signs of major mergers or tidal disturbances, there may be minor asymmetries or faint features hinting at past interactions. Overall, the galaxy appears to be a relatively massive system undergoing moderate levels of star formation, with a color gradient suggesting radial variations in stellar population ages.
