The galaxy presents as a relatively smooth, elliptical-like structure. There is a noticeable concentration of light towards the center, suggesting a bulge. The galaxy's overall color appears to be slightly redder, which could indicate an older stellar population with a lower rate of star formation. No spiral arms or distinct features are readily apparent in this image. The galaxy exhibits a fairly regular, rounded morphology. There is no obvious evidence of recent or ongoing major merger activity, though some minor disturbance cannot be ruled out based on this single image alone.
