The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, centrally bright morphology with a gradual decrease in luminosity towards its outer regions. The color profile indicates a redder overall hue, suggesting an older stellar population and a relatively low rate of ongoing star formation. There is a slight elongation observed, but it is generally round in appearance. No prominent spiral arm structures or dust lanes are discernible. The galaxy does not display any obvious signs of major mergers or tidal disturbances, although subtle asymmetries in the outer halo cannot be entirely ruled out given the image quality. The overall structure suggests a gravitationally relaxed system approaching quiescence.
