The galaxy presents an elongated, cigar-shaped morphology. It exhibits a predominantly smooth appearance overall, though there's some suggestion of finer structure within. A central, brighter region appears to be present, potentially indicative of a galactic bulge. The color profile shows a gradient, with bluer hues concentrated at the edges. This might suggest ongoing star formation in the outer regions. There also appear to be redder regions distributed along the galaxy. These likely indicate older stellar populations, or possibly dust extinction. There may be minor distortions within the galaxy. These could potentially suggest past interaction with another galaxy, or internal dynamics at play.
