The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. There is little evidence of spiral arm structure or prominent disk features. The color profile suggests an older stellar population, with a yellow-red hue dominating. This color is generally indicative of galaxies where star formation has slowed or ceased. The galaxy appears fairly isolated, with no immediate signs of major interaction or tidal disruption. There is a slight deviation from perfect circularity in the morphology. Though mostly smooth, some subtle perturbations might be present within the galaxy's outer regions.
