The galaxy appears as a diffuse, elliptical object with a relatively smooth profile. The light distribution is concentrated towards the center, with a gradual decrease in brightness toward the outer regions. There are subtle variations in color, with a hint of bluer hues near the center, potentially indicating regions of younger stars or active star formation. The galaxy exhibits a slightly elongated shape. No distinct spiral arms or prominent dust lanes are discernible. There appears to be some degree of asymmetry or minor disturbance in the overall structure.
