The galaxy presents a distinct, elongated morphology, approximating a cigar shape. Its luminosity profile appears relatively smooth and centrally concentrated, with a gradual decrease in brightness extending outwards from the core. There is a faint blue hue, possibly indicative of some ongoing, albeit low, star formation activity. No prominent spiral arm structures or significant dust lanes are discernible in this image. The galaxy lacks any clear signs of major mergers or tidal disturbances. The overall appearance suggests a quiescent system.
