The galaxy appears to be a relatively bright, elongated object. A concentrated central bulge or core is visible, exhibiting a yellowish hue. This suggests the presence of an older stellar population within the core. Fainter, somewhat diffuse disk-like structures extend outward from the central region, showing hints of spiral arm morphology. The disk component displays a bluer color compared to the central bulge, which may indicate ongoing star formation within the disk. There is a possible small companion galaxy or star forming region in the bottom left corner of the image. Based on morphology, there are no obvious signs of a major ongoing merger, although a slight asymmetry in the disk could indicate a past interaction.