The galaxy presents as a somewhat irregular, luminous structure. A dominant, centrally located, roughly spherical component is visible. This component has a smooth texture and a somewhat diffuse edge, indicating potentially an elliptical morphology. Additionally, there is evidence of possible tidal disturbance; this can be seen from the slightly distorted shape of the disk-like component of the galaxy and faint plume-like features extending away from the main body. Color gradients across the galaxy suggest varying stellar populations, with bluer regions potentially indicating ongoing star formation and redder regions potentially indicating older stellar populations.
