The galaxy appears to be a relatively smooth, elliptical-like structure. The core region displays a bright, concentrated luminosity, appearing a yellow-orange hue. The light gradually decreases in intensity towards the outer regions, showing a diffused halo with a slightly bluer tint. There is no visible spiral arm structure or obvious dust lane obscuration. There is little morphological disturbance apparent within the galaxy, indicating it is likely not undergoing major merger activity. The generally smooth appearance and color suggest that the galaxy is primarily composed of older stellar populations, with a limited current star formation rate. Overall, this galaxy appears to be a mature, relatively quiescent system.
