The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. The light profile indicates a relatively high degree of central concentration. It is elongated in shape, with a cigar-like appearance. The color indices suggest a relatively old stellar population, giving it a yellow hue. There is no obvious evidence of ongoing star formation or spiral arm structure. Additionally, there are no clear signs of any recent or ongoing merger activity or major disturbances within the galaxy's structure.
