The galaxy exhibits a morphology indicative of a possible ongoing merger event or strong tidal interaction. The primary body of the galaxy appears to be somewhat amorphous, with a central concentration of light and diffuse outer regions. There is a distinct, bright, compact core. The light from the galaxy is dominated by bluish and white hues, suggestive of a relatively high population of young, hot stars or potentially an active galactic nucleus. There are hints of faint, reddish regions on the outer edges of the galaxy, which could indicate older stellar populations or dust lanes. Overall, the galaxy's structure shows a combination of smooth, centrally concentrated light and potentially disturbed features.
