This galaxy exhibits a generally smooth morphology, with an elongated, cigar-like shape. The galaxy appears to be undergoing a merger or strong tidal interaction, as evidenced by the distinct double nucleus or highly disturbed core. The color distribution is relatively smooth, with a yellowish hue dominating the central region, which may indicate an older stellar population. The galaxy shows some evidence of possible disruption in its outer regions, though the overall structure suggests a transitioning stage within a merger event. The image resolution does not allow for a detailed assessment of any spiral arm structure or dust lanes.
