The galaxy presents a somewhat elliptical morphology. Its central bulge is bright and appears relatively smooth. The surrounding disk exhibits a bluer hue, suggesting the presence of ongoing star formation. There are hints of subtle disturbances within the disk, such as faint, irregular structures. The overall color profile indicates a galaxy with a mix of older stellar populations in the bulge and younger, actively forming stars within the disk. There isn't a clear, grand spiral arm structure.
