The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and featureless morphology. The light distribution is concentrated towards the center, suggesting a prominent galactic bulge. The galaxy exhibits a moderate roundness, with no significant elongation or distortion apparent in the image. There is no visually discernible evidence of spiral arms, bars, or tidal tails. The color profile indicates a concentration of older stellar populations, given the observed redder hues dominating the central regions, transitioning to relatively bluer hues further out. No significant dust lanes or active star forming regions are directly observable. The overall impression is of a passively evolving galaxy. There is no evidence of a major ongoing merger event, though minor disturbances can't be ruled out.
