The galaxy presents as an elongated, cigar-shaped morphology, likely a flattened elliptical or potentially an edge-on spiral galaxy. The light distribution appears relatively smooth and centrally concentrated. A subtle color gradient is visible, transitioning from a bluish hue in what might be the outer regions to a slightly redder color toward the central bulge. This color variation could indicate differing stellar populations or dust content across the galaxy. There is little evidence of distinct spiral arm structure or significant star-forming regions based on the image. No signs of recent or ongoing major merger events can be seen, such as tidal tails or highly disturbed morphology, but there is a slight disturbance in the disk.
