This galaxy appears to be in a state of interaction, potentially a merger. The overall structure is irregular and elongated, showing signs of tidal distortion. A prominent feature is the brighter, somewhat compact core region, which exhibits a yellowish hue, suggesting an older stellar population or significant dust obscuration. Extending outwards from the core is a fainter, bluish arm-like structure, indicating regions of more recent star formation. At least one distinct tidal tail can be observed, exhibiting a diffuse, bluish color, indicative of young stars formed as a result of the gravitational interaction. There may be a second possible core, indicating that this might be a merger. The overall light profile is complex, with no clear evidence of a regular spiral or elliptical morphology. There are also other blueish regions besides the arms, suggesting pockets of active star formation.
