This galaxy presents an elongated, cigar-shaped morphology. The central region appears bright and smooth, indicative of a high concentration of stars likely associated with an older stellar population. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to more reddish hues at its periphery, which could suggest variations in stellar populations or dust content. There are no prominent spiral arms or bar structures visible. A subtle, asymmetrical extension is observed on one side of the galaxy, potentially indicating a minor gravitational interaction or tidal feature, though a more in-depth spectroscopic analysis would be required to confirm the galaxy's morphology and evolutionary state. The galaxy appears relatively undisturbed with no major mergers occurring. Overall, the galaxy seems to be in a state of low to moderate star formation.
