This galaxy presents an interesting morphological structure, potentially indicative of an ongoing or recent merger event. The overall shape is not particularly well-defined, with some apparent disturbances in its morphology. It exhibits an extended, diffuse component with a less concentrated central region.

There appears to be two distinct nuclei within the galaxy, suggesting a possible interaction or merger between two separate galaxies. The dominant component displays a bulge with moderate brightness, while the secondary component is more compact and appears brighter.

In terms of color, there is some variation across the galaxy, suggesting differing stellar populations. The central region of the main component appears more yellow in color, potentially indicating an older stellar population. The outskirts of the galaxy and the secondary component show bluer regions that suggest recent or ongoing star formation. Overall the specific star formation rate seems relatively low.
