The galaxy presents a generally smooth and rounded morphology. There is a concentrated central bulge that transitions smoothly into the outer regions of the galaxy. There is a slight color gradient, with the central region exhibiting a yellowish hue that may indicate an older stellar population. The outer regions appear to be composed of a faint disk. There is a slight hint of a spiral structure, but this cannot be stated with certainty. The galaxy does not appear to be undergoing any major mergers or interactions.
