This galaxy appears as a relatively smooth, disk-shaped object, exhibiting a slight inclination relative to our line of sight. Its overall color suggests a mix of stellar populations, with a central region that is more red or orange, potentially indicating an older stellar population. The outer regions of the galaxy display a distinct green or blue tint, hinting at the presence of younger, hotter stars and ongoing star formation. There is no strong evidence of spiral arm structure, though subtle variations in color and brightness might suggest faint, ill-defined features within the disk. Overall, the galaxy appears relatively isolated and undisturbed, showing no obvious signs of major interactions with other galaxies or significant morphological disruptions. The galaxy's apparent size and shape indicate that it could be an average-sized spiral or lenticular galaxy at a moderate distance.
