This galaxy appears to be an elliptical galaxy, with a relatively smooth and featureless morphology. There is a slight elongation to the structure, suggesting it is not perfectly spherical, tending towards a more lenticular or cigar shape. The color profile indicates an older stellar population, with a reddish hue overall, implying a lower rate of star formation. Based on its apparent smoothness and color, it likely contains a significant population of evolved stars and potentially a supermassive black hole at its center. There is some sign of possible tidal disruption, so either there has been a past merger, or it is ongoing.
