The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The core exhibits a high surface brightness, concentrated towards the center. The galaxy appears somewhat elongated, deviating from a perfectly circular shape; it has a cigar-like appearance. There is no discernible spiral arm structure or distinct dust lane features. The color gradient suggests a population of older stars, with a redder hue dominating the galactic body. There are no obvious signs of any major ongoing merger activity.
