The observed galaxy presents as a disk galaxy, viewed at a high inclination. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population. The disk component appears flattened and elongated. There is a bluer color along the edges of the disk indicating a younger stellar population, possibly regions of active star formation. Overall, the galaxy seems to be well-defined, with a smooth distribution of light and no major signs of tidal disturbance.
