The galaxy presents as a relatively smooth, disk-like structure. Its morphology indicates a system that is mostly undisturbed, showing little evidence of major mergers or significant tidal interactions.

The galaxy's color gradient suggests a centrally concentrated older stellar population and a star forming disk component. The core exhibits a bright, concentrated region likely corresponding to a galactic bulge with aging stars. The surrounding disk shows a bluer hue, suggesting ongoing star formation.

There might be some minor disturbance visible in the galaxy's shape, though the galaxy's overall structure is not highly irregular.

Overall, this galaxy appears to be an intermediate-mass disk galaxy with a moderate level of ongoing star formation and a dominant bulge component.
