The galaxy presents a relatively smooth and centrally concentrated morphology. It exhibits a largely elliptical shape, showing a gradient in luminosity from the center to the outer regions, indicating a bulge-dominated system. There is little evidence of spiral arm structure or significant dust lanes within the galaxy. The primary color gradient moves from a golden hue in the galactic center to a cool blue in the outer parts. The galaxy appears to be a mature system, exhibiting a population of older stars contributing to its reddish color, with some evidence of ongoing star formation in bluer outer regions. There is no discernible indication of tidal features or interactions with neighboring galaxies. The galaxy is fairly well-isolated.
