The galaxy presents as an elongated, cigar-shaped structure. The primary body exhibits a yellowish-orange hue, indicative of an older stellar population. A brighter, slightly blueish disk is visible, suggesting ongoing star formation, albeit relatively muted compared to the older population. There is possible evidence of tidal disturbances or merging activity. Although not clearly defined, there is a faint trail towards the lower region, which indicates gravitational interaction with another object, possibly the remnant of a merger. Based on the color gradients and morphology, the galaxy appears to be a disk galaxy undergoing a merger.
