The galaxy appears to be a relatively compact system with a slightly elliptical morphology. A central bulge is visible, characterized by a reddish hue, suggesting an older stellar population. Fainter bluish light extends outwards from the central region, potentially indicating the presence of younger stars and ongoing star formation within a disk-like component. There are hints of faint spiral arm structures, but they are not well-defined. No obvious signs of a major merger are apparent, though some minor disturbances cannot be ruled out based on this image alone.
