The galaxy presents a relatively smooth, centrally concentrated morphology. Its shape is close to round with very little elongation and no obvious distortions suggestive of a recent major merger event. The dominant color is a mixture of blue and green, implying the presence of some younger, hotter stars undergoing active star formation. The redder halo implies the galaxy contains an older stellar population. The smooth features, color and spherical morphology are suggestive of a disk galaxy, possibly seen nearly face-on.
