The galaxy presents an elongated, disk-like morphology, appearing nearly edge-on from our perspective. The central region exhibits a concentrated bulge, characterized by a yellowish-white hue, suggesting a population of older stars. The disk component displays a gradient of color, transitioning from greenish-blue closer to the core to reddish tones at the outer edges. This color variation suggests varying stellar populations within the disk, with bluer regions potentially indicating ongoing star formation. The overall structure appears relatively undisturbed, showing no obvious signs of recent major mergers, though subtle irregularities in the disk could indicate minor gravitational interactions. The estimated size of the galaxy indicates it is a sizable object. The redshift indicates it is not particularly far away.
