The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. The main body appears somewhat smooth but with a notable, elongated structure, suggesting a disk component viewed at an oblique angle. The color is predominantly bluish, indicating the presence of relatively young, hot stars and active star formation. There are faint diffuse features extending from the central region, possibly tidal tails or disrupted arms. These suggest gravitational interactions with another galaxy. The distribution of light is not uniform, with a brighter core region and a gradual decrease in intensity outwards, consistent with a central bulge or nucleus. The shape appears significantly distorted from a regular elliptical or spiral form, lending further support to the hypothesis of a merging system or recent interaction.
