The galaxy presents as a moderately sized object with a centrally concentrated light profile. The main body of the galaxy appears largely smooth in texture. There is no obvious spiral arm structure visible. The color gradients show a blue-white hue in the central region, which might indicate a higher concentration of younger, hotter stars. Towards the outer regions, the color shifts towards redder and yellow tones, potentially suggesting an older stellar population. There appears to be some signs of minor interaction or disturbance within the galaxy system, but mostly the galaxy remains relatively smooth. The morphology suggests a relatively passive evolution, although recent or ongoing minor merger events cannot be ruled out based on this image alone.