This galaxy presents an interesting morphology, appearing to be a system undergoing a significant interaction, possibly a merger. It exhibits a distinct, elongated tidal tail extending from the primary galactic body toward the west. This tail displays a yellowish hue, suggesting a population of older stars and possibly dust.

The main body of the galaxy appears disturbed. There is a brighter, more concentrated region within it, displaying a white-blue color, indicative of younger, hotter stars. This might signify a region of enhanced star formation triggered by the interaction. The overall structure of the galaxy lacks a well-defined spiral or elliptical form, further supporting the hypothesis of a system experiencing a disruptive event. There is a hint of redder regions interspersed within the galaxy's body, which could be indicative of dust lanes or areas of ongoing star formation embedded within dust clouds. The galaxy’s light profile is relatively diffuse, which is in line with a higher redshift. The interaction appears significant enough to disturb the overall morphology and trigger enhanced star formation.
