The galaxy appears to be a relatively smooth, elliptical-like object. It presents with a somewhat elongated morphology, displaying a cigar-like shape. The light distribution indicates a central concentration of luminosity that decreases gradually outward, suggesting a dense core region. There is no discernible disk-like structure or prominent spiral arms. The galaxy exhibits a yellow-white hue in the image, suggesting a population of older stars. No major disturbances or signs of an ongoing merger are evident.
