The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. A dominant central bulge is visible, exhibiting a concentrated, bright yellowish hue suggesting an older stellar population. There are no obvious spiral arm structures. The overall color profile indicates a redder, more evolved system, with only faint hints of bluer star formation regions. Minor distortions are possibly present in the outer halo but the signal is extremely faint. The galaxy is generally isolated, showing minimal signs of tidal interaction or merging events with nearby galaxies, but appears to possibly be attracting a smaller, less dense structure.
