The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. Its shape deviates from a perfect sphere, showing some elongation; it is cigar shaped. The light distribution suggests an older stellar population with a yellowish hue. There is no clear evidence of spiral arms or a prominent disk. There is no major galaxy merger, but the morphological analysis indicates a non-zero probability of a minor disturbance. The galaxy is relatively compact.
