The galaxy presents an elongated morphology, appearing approximately 0.8 kpc in diameter. It exhibits a pronounced arc-like structure with multiple distinct luminous regions. Color variation is apparent along the galaxy's length, with one end displaying a yellow-orange hue that transitions to a bluer tint at the opposite end. The observed color gradient suggests varying stellar populations. Some regions appear more actively star-forming. There is an indication of tidal interactions and mergers in its recent history, with significant disturbances or mergers in progress. The main body of the galaxy shows no clear spiral structure or well-defined disk; instead, the light distribution is relatively smooth. Overall, the galaxy appears to be in an advanced state of interaction, leading to an irregular shape and possible bursts of star formation activity.
