The galaxy appears to be undergoing some form of disturbance. A notable feature is the presence of a brighter, somewhat compact central region, potentially a bulge. Surrounding the central area is a less defined, more diffuse region exhibiting a bluer hue, possibly indicating ongoing or recent star formation. The primary body exhibits a more smoothed appearance with what appears to be a slight flattening or extension along one axis. The galaxy does not display a strong spiral arm structure. There is evidence of minor disturbances in the overall symmetry and morphology.
