The galaxy presents as a disk-shaped system, elongated in appearance. The central region exhibits a more concentrated and brighter luminosity, possibly indicating a bulge component. The color gradient suggests a primarily older stellar population concentrated in the center and disk with regions of ongoing or recent star formation toward the edges. The galaxy appears to be relatively undisturbed, showing no strong signs of major mergers or tidal interactions. Overall, it seems to be a disk galaxy viewed at an angle.