This galaxy exhibits a generally smooth morphology, suggesting it is likely an elliptical or lenticular type. The light distribution appears highly concentrated towards the center, indicating a prominent galactic bulge. The galaxy presents a nearly round shape, with only slight deviations from perfect circularity. There is no discernible spiral arm structure or a defined disk component evident in this image, though faint disturbances appear around the body. The galaxy exhibits a broad color gradient, with the central region appearing more yellowish, possibly indicating an older stellar population with diminished recent star formation. The outer regions appear slightly bluer, though this could also be the product of image noise. No obvious signs of ongoing major mergers are present.
