The galaxy exhibits an overall elongated, cigar-shaped morphology. It is composed of two distinct components, likely interacting. The first component appears as a bright, relatively smooth and amorphous structure with a blue-ish hue, potentially indicative of a population of young, hot stars or significant ongoing star formation. This feature dominates the blue light. The second component, positioned below the bluer one, is more disk-like, with a yellowish-gold color, suggesting an older stellar population. There is a hint of possible tidal disturbance or interaction, but it is difficult to ascertain significant merger activity based solely on the image. The galaxy appears relatively compact. The smoother, bluer component exhibits slightly more dominant light than the other.
