This galaxy presents as an elongated, cigar-shaped structure, suggesting an elliptical morphology. The core exhibits a concentrated, brighter region, indicative of a higher stellar density. The galaxy appears smooth with no readily discernible spiral arm structures or significant dust lanes. The color gradient transitions from a yellowish-white core to a redder hue in the outer regions, which may imply an older stellar population at the center and relatively younger stars in the outer regions. There's no obvious sign of an ongoing merger, though very minor disturbances cannot be ruled out at this resolution. The overall form suggests a relatively evolved galaxy with a substantial stellar mass and a moderate rate of star formation. The light distribution indicates a generally symmetric structure, consistent with a settled system.
