The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated morphology. It presents as elongated, cigar-shaped. There is a central bulge that is bright yellow-orange, indicating a population of older stars. No distinct spiral arms or disk-like structures are visible. The overall color suggests a relatively low rate of star formation. The galaxy may be undergoing or have undergone a merging event, but it is difficult to tell with certainty.
