The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with no discernible spiral arms or prominent disk structure. The galaxy's light profile suggests a concentrated central bulge, gradually fading outwards. Its color is predominantly yellow-orange, indicating an older stellar population and reduced ongoing star formation. There is no significant dust obscuration visible, suggesting that the galaxy is relatively quiescent. The galaxy displays a fairly regular shape, with no apparent tidal features, distortions, or signs of recent or ongoing merger activity. The absence of blue light suggests a lack of young, hot stars and active star formation, aligning with a more evolved galaxy with a large stellar mass and a low specific star formation rate.
