This galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical light distribution with a highly concentrated central region, likely a galactic nucleus. The galaxy displays a golden hue, suggesting a relatively old stellar population, with less ongoing star formation. The elliptical shape shows a moderate degree of ellipticity. There is no clear evidence of spiral arms or a prominent disk. The galaxy appears relatively isolated, showing no obvious signs of tidal disruption or interaction with neighboring galaxies. The general morphology suggests a well-evolved, early-type system.
