The galaxy presents an elongated, cigar-shaped morphology. It exhibits a relatively smooth appearance, suggesting a lack of significant spiral arm structure or prominent dust lanes. The central region appears brighter and more concentrated, possibly indicating the presence of a galactic bulge. A subtle color gradient is observed, with the central region appearing slightly more blue, possibly indicating recent star formation activity, while the outer regions show a redder hue. There are no signs of major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out. Overall, this appears to be a relatively evolved galaxy that may be undergoing a period of quiescence in terms of star formation.
