The galaxy exhibits a lenticular morphology, presenting a flattened disk-like structure. A bright, prominent central bulge is clearly visible, appearing almost spherical and intensely luminous. This suggests a high concentration of stars within the galactic nucleus. Surrounding the bulge is a fainter, more diffuse disk component. There are no discernible spiral arms or bar-like structures within the disk. The overall color of the galaxy leans toward a blue-green hue, more concentrated around the central bulge, which could indicate active star formation regions within or around the bulge. However, the surrounding disk appears slightly redder in comparison, possibly due to the presence of older stellar populations or dust obscuration. The galaxy appears to be relatively isolated with no nearby companion galaxies evident in the immediate vicinity, although there is the suggestion of a very minor tidal disturbance.
