The galaxy presents as a disk-shaped structure, viewed nearly edge-on from our perspective. A prominent central bulge is observed, appearing bright and yellowish in color, suggesting an older stellar population. The disk itself exhibits a more subdued, mottled appearance, with hints of blueish regions intermixed with dust lanes. These features are consistent with ongoing, but not necessarily vigorous, star formation. There are no indications of a major merger event, although subtle disturbances or faint tidal features cannot be definitively ruled out at this resolution. Overall, the galaxy appears to be a relatively isolated system in a state of established dynamical equilibrium.
