The galaxy presents an irregular morphology, displaying evidence of ongoing or recent interaction or merger activity. A prominent feature is a bright, compact region exhibiting a bluish hue, suggestive of a concentrated area of recent star formation. This region contrasts with a separate, more diffuse area displaying a yellower/redder color, indicating an older stellar population or the presence of dust obscuration. The galaxy lacks a clearly defined spiral structure or elliptical shape, which further supports its classification as an irregular system potentially undergoing a merger. Faint tidal features may be present, but the image quality limits definitive identification. The overall color suggests a moderately active star formation rate, with the blue region indicating a localized burst of activity.
