The galaxy exhibits a generally smooth morphology, with a dominant central bulge that appears approximately oblate in shape. The ellipticity suggests it is not perfectly spherical. There is a faint, diffuse disk-like structure surrounding the bulge. The color gradient indicates a concentration of older stellar populations in the central bulge, which displays a yellowish hue. The outer disk region shows a slight bluer tint, potentially indicating the presence of younger, hotter stars, even though the overall star formation rate appears low. There is no indication of major spiral arms or strong bar features; however, there appears to be a minor disturbance and potential sign of a smaller galaxy nearby, but this may also be a feature internal to the disk.
