The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light profile appears relatively smooth and concentrated toward the center, suggesting a bulge component. There is an apparent absence of well-defined spiral arms, indicating a possible classification towards elliptical, or perhaps a lenticular galaxy seen edge-on. The color appears to shift from red on one end to bluer hues near the opposite end and within the central region, implying a potential gradient in stellar populations or dust content across the galaxy. Overall, the galaxy appears to be generally undisturbed, lacking any obvious signs of recent major mergers or interactions, with only a hint of minor disturbance.
