The galaxy presents an elliptical morphology with a centrally concentrated bulge. The bulge exhibits a yellowish hue, indicating a population of older stars. A faint, flattened disk surrounds the bulge, displaying a bluer color suggestive of younger, hotter stars and potential ongoing star formation. The disk appears relatively smooth, with no prominent spiral arm structures readily discernible in the image. Overall, the galaxy appears to be a relatively undisturbed system, with a slight tilt relative to our line of sight.