The galaxy presents as an elongated structure with a noticeable disruption in its morphology. A significant concentration of light is observed on the right side of the galaxy. This area has a bluer hue, suggesting a high concentration of younger, hotter stars, possibly indicating recent or ongoing star formation. The light appears fairly centralized, making it hard to determine if there are any distinct spiral arms within the galaxy, suggesting that it is more spheroid or diffuse. A faint tail or bridge of stellar material extends to the left, which might be the result of tidal interactions with another celestial body. The central region of the galaxy appears to be somewhat blended with this extended feature. Overall, this galaxy appears disturbed and not fully resolved.
