The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. Its overall shape appears to be moderately round, without any obvious signs of significant disturbance or ongoing merger activity. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central regions. A slight extension of the isophotes along one axis hints at a flattened, ellipsoidal structure. No distinct spiral arms or prominent dust lanes are visible within the image resolution. The general morphology suggests a system that has largely completed its major star formation phase, and is currently dominated by evolved stars.
