The galaxy exhibits an elliptical morphology, appearing mostly smooth and featureless. There is a concentration of light towards the center, suggesting a prominent galactic nucleus or bulge. The isophotes are generally elliptical, showing a moderate ellipticity. The color gradient indicates a yellow to red central region and slightly bluer outer regions, suggesting older stellar populations in the core and ongoing star formation in the disk. Based on its visual appearance, there's a possible minor disturbance, though a well-defined tidal tail is absent. No clear evidence of a major merger is visible from this image. The galaxy appears to be of significant mass and luminosity.
