The observed galaxy presents as a disk galaxy viewed nearly edge-on. A prominent bulge dominates the central region, exhibiting a smooth, rounded morphology with an orange hue. This suggests a large population of older stars. The galactic disk appears as a flattened structure extending from the central bulge. Dark dust lanes are not clearly visible, indicating a relatively low dust content. The disk displays a faint bluish tinge in the outer regions. This suggests the presence of younger, hotter stars contributing to a moderate level of star formation. There are no obvious signs of strong tidal disturbances or interactions with other galaxies.
