The galaxy presents a generally smooth, elliptical morphology. There is no clear evidence of spiral arm structure or a prominent disk. The light distribution appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. The galaxy exhibits a yellowish-orange hue throughout, suggesting an older stellar population, likely dominated by evolved stars. There are no distinct blue regions indicative of active star formation apparent in this image. Overall, the galaxy appears to be a relatively undisturbed system with no signs of major mergers or tidal interactions.
