The galaxy presents as a somewhat elongated structure with a relatively smooth appearance. A central bulge is visible, appearing brighter and more concentrated than the surrounding regions. This bulge exhibits a slightly yellowish hue, which suggests a population of older stars. The disk component of the galaxy, surrounding the bulge, displays a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. There appears to be some disturbance in the disk, as the disk is asymmetrical and doesn't have clear spiral arms or banding. Despite this disturbance, there is no obvious sign of a major ongoing merger. This galaxy appears to be a disk galaxy, potentially with a suppressed or irregular spiral structure. 
