This galaxy appears to be a relatively smooth and round object, with a concentrated central region indicating a prominent bulge. There is little evidence of spiral arms or distinct features beyond the overall elliptical shape. The color gradient transitions from a yellowish-white core to a reddish-tinged outer halo, possibly indicating a difference in stellar populations, with older, redder stars populating the outer regions and younger, bluer stars concentrated towards the center. The galaxy exhibits a low level of star formation activity. There is no evidence of a major ongoing merger, tidal distortions, or significant disturbances in the overall structure.