The galaxy appears as a singular, centrally concentrated object. It exhibits a smooth, elliptical morphology with no apparent spiral arm structures. The light distribution is relatively uniform, with a gradual falloff in intensity from the core to the outer regions. The galaxy is quite round in appearance. A slight color gradient is noticeable; the core presents a yellow-gold hue, suggesting an older stellar population, with a subtle shift toward redder colors in the outskirts, which may indicate the presence of dust. There is no evidence of ongoing major mergers or tidal disruptions in this image, though minor disturbances cannot be ruled out at this resolution. Overall, it is a relatively quiescent, evolved galaxy.
