The galaxy presents a generally smooth and rounded morphology. It appears largely featureless upon visual inspection, showing a centralized concentration of light that diminishes gradually towards the edges. The galaxy's color profile suggests an older stellar population; the core exhibits a yellow-orange hue, indicative of evolved stars, while the outer regions display a slight blue tinge, hinting at trace amounts of ongoing or recent star formation. There is no discernible evidence of spiral arms or a pronounced disk structure. It does not appear to be undergoing any major merger events, although minor disturbances cannot be entirely ruled out.
