The galaxy appears to be undergoing a significant interaction, possibly a merger. The overall morphology is disturbed, with a notable lack of defined spiral arms or a smooth elliptical shape. There are at least three distinct luminous components, with the brightest appearing yellow, perhaps indicative of an older stellar population. A smaller, bluer component suggests more recent star formation activity. A third, more diffuse, component is present, exhibiting a mix of colors, which may be tidal debris or stars scattered during the interaction. The galaxy does not have a well-defined central bulge or disk, further supporting the hypothesis of a merger in progress. Overall, the galaxy presents a complex and dynamically active system.
