The galaxy presents a generally smooth appearance, with a slight elongation in its overall shape. The central region appears more concentrated and brighter than the outer regions, suggesting a bulge. There is evidence of some minor disturbances in the disk region, such as slight asymmetries in the shape or distortions in the arms. The color profile suggests that there is active star formation occurring within the galaxy, as indicated by the presence of a bluer color in the outer disk areas. The galaxy's morphology appears to be transitioning between a fully elliptical system to a spiral galaxy with a more complex structure.
