This galaxy presents an elongated, disk-like morphology, viewed at a significant inclination. The central bulge region exhibits a concentrated, yellowish hue suggesting an older stellar population. Extending outward from the bulge, the disk shows a bluer color gradient, possibly indicating ongoing or recent star formation. The disk appears relatively smooth and uniform, with no prominent spiral arm structures immediately apparent. The edges of the disk are somewhat diffuse, indicating potential tidal interactions or a gradual decrease in stellar density. No significant signs of major mergers or violent disturbances are readily visible, although subtle features or minor disturbances cannot be ruled out at this resolution. The galaxy appears moderately massive and is undergoing some level of star formation activity.
