This galaxy appears to be a disk galaxy, observed nearly edge-on. A central bulge is visible, displaying a relatively smooth and bright morphology. A flattened disk extends outwards from the bulge, though it appears relatively faint and lacks distinct spiral arm structures. There may be hints of dust lanes obscuring parts of the disk. Based on its color, it might be experiencing some star formation activity, although the rate seems relatively low. There is some indication of minor disturbance in the galaxy's structure, such as warping or tidal features. The image suggests that it is not a strong merger, but may have interacted with other galaxies in the past. Overall, the galaxy exhibits a morphology consistent with a disk galaxy in a relatively quiescent state.
