The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The galaxy exhibits a generally round shape. There is some evidence of minor disturbances in the galaxy's structure, potentially indicative of a past or ongoing interaction. The galaxy displays a color gradient, with a bluer hue towards the center transitioning to redder tones in the outer regions. This may be caused by the varying ages and compositions of the stellar populations. Star formation appears to be ongoing, albeit at a relatively low rate, based on the color profile. The mass of the galaxy is substantial, suggesting an established stellar population.