This galaxy presents an intermediate morphology, appearing to be between a spiral and an elliptical type. The light distribution is centrally concentrated with an apparent bulge component. There is evidence of a faint, flattened disk extending beyond the central bulge, although the disk is relatively smooth and lacks clearly defined spiral arms. The overall color suggests an older stellar population, with a reddish-yellow hue dominating the light emitted. There are only slight color variations observed across the galaxy, with the central region appearing somewhat yellower. This is possibly due to an increased density of older stars towards the galactic center. There is no visual evidence of recent star formation. The galaxy appears relatively undisturbed with no major tidal features or distortions suggesting recent mergers, although the presence of some minor disturbances can not be ruled out given the images resolution.
