The galaxy presents a generally smooth morphology with a concentrated central bulge. The light distribution is relatively uniform across the main body, but it exhibits a slight elongation. There appears to be some mild distortion, possibly indicative of a minor gravitational interaction or disturbance. The galaxy's color suggests a mix of stellar populations with a slightly redder hue at the edges, indicative of an older population of stars. A brighter, yellow central region could indicate a younger, hotter population, or increased activity in the galactic core. The overall structure lacks strong spiral arms, and does not have a clear disk shape. 
