The galaxy presents a slightly elongated morphology, appearing as a disk galaxy seen at an oblique angle. There is evidence of some internal structure, although it is somewhat indistinct. A central bulge is visible, surrounded by a disk with hints of spiral arm structure. The color gradient suggests ongoing star formation. The inner regions appear slightly redder, potentially indicating an older stellar population, while bluer hues in the outer disk imply younger, hotter stars. The galaxy does not show significant signs of major disturbances. There is some irregularity on the left side that could be signs of a minor merger or tidal interaction, possibly contributing to the observed star formation.
