The galaxy appears to be a disk galaxy, viewed at a high inclination. There is evidence of a central bulge that is bright and yellow-white in color. Around the bulge, a ring-like structure is visible, exhibiting a mix of colors, from blue to green, and red. The color suggests active star formation within this ring. The galaxy shows subtle signs of disturbance, possibly due to a minor merger or tidal interaction, as hinted by the slight asymmetry observed and the presence of faint, extended light around the primary structure. There may also be a faint spiral structure extending out beyond the bright central region, however, it is too indistinct to say for certain. Overall, the galaxy's morphology suggests an intermediate stage of galactic evolution, possibly involving recent or ongoing interactions affecting its star formation and structure.
