The galaxy presents as a moderately inclined disk, with a clearly defined central bulge region. The light distribution suggests a relatively smooth stellar population throughout the disk, though with some subtle variations in color and intensity. The bluish hue along the disk indicates the presence of younger, hotter stars, implying recent or ongoing star formation, particularly concentrated within the disk. The edges of the disk appear somewhat diffuse, potentially due to dust obscuration or the gradual decrease in stellar density at the galaxy's periphery. There are no immediately obvious signs of strong spiral arm structure or a prominent bar feature within this image, though finer details might be unresolved at this resolution. The bulge appears more yellow or white, which could indicate an older stellar population. There is no evidence of any major ongoing merger events.
