The galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests a fairly elliptical morphology, exhibiting a high degree of roundness. There is a central, luminous core that gradually fades outward, lacking any distinct spiral arm structure or prominent features such as dust lanes or knots of star formation. The galaxy has a yellow-ish color, suggesting an older stellar population with suppressed star formation. There is no visual evidence of ongoing or recent major merger events, although minor disturbances cannot be ruled out based solely on the image.
