The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It has a slightly elongated morphology, with a cigar-like shape. There are no obvious signs of spiral arms or a prominent disk structure. The galaxy presents a fairly symmetrical profile, lacking any apparent major disturbances or merger events. The color gradient suggests a higher concentration of older stellar populations toward the center of the galaxy, with bluer hues possibly indicating some ongoing star formation. The galaxy is relatively compact, with a size of a few kiloparsecs.
