The galaxy appears as a relatively small, well-defined object with a noticeably flattened, disk-like morphology. It presents a smooth appearance overall, with a high degree of central concentration. The inner regions exhibit a bright, almost amorphous glow that may consist of older stars. The outer regions are more diffuse and less luminous, showing a clear transition from the concentrated central bulge to a fainter halo.

The color distribution indicates an increased concentration of younger, star forming regions that extend around the inner areas of the galaxy. This suggests the presence of ongoing star formation. The galaxy does not appear to be undergoing any major mergers, with no prominent tidal tails or distorted features visible. It shows some minor disturbances suggesting minor gravitational interactions. In summary, it appears to be a relatively isolated disk galaxy, potentially an early spiral or lenticular galaxy.
