The galaxy presents a largely smooth morphology. Its light is concentrated centrally in a bright, nearly circular core, fading gradually outward. The central region exhibits a yellowish-orange hue, suggesting an older stellar population with limited ongoing star formation. The outer regions display hints of a more diffuse, bluish-green color, which may indicate some presence of younger, hotter stars, although it could also result from the averaging of the color data. There appears to be minimal evidence of spiral arm structure or significant tidal disturbances; the image shows no clear indication of a merging event. Overall, the galaxy appears to be a relatively quiescent system, likely an elliptical or lenticular type.
