This galaxy presents as an elongated structure, likely a disk galaxy viewed nearly edge-on. A prominent central bulge is visible, appearing smooth and rounded. The bulge exhibits a yellowish hue, suggesting a population of older stars. The disk component appears relatively smooth. A slight blueish tint extends from the disk, indicating regions of younger stars. The galaxy appears to be relatively undisturbed, without signs of a recent major merger or tidal interactions. The overall morphology suggests a massive galaxy with a low star formation rate.
