The galaxy presents an elongated, cigar-shaped morphology. It appears largely smooth with a dominant central bulge. There is a color gradient evident across the galaxy, with the central region exhibiting a more reddish hue, possibly indicating an older stellar population or dust obscuration. The outer regions show a slight bluer tint, suggesting the presence of some younger stars or ongoing star formation, although overall, it's not intensely active. No signs of major mergers or tidal disturbances are readily apparent. The galaxy seems relatively isolated and undisturbed.
