The galaxy presents as an elongated, disk-like structure oriented approximately vertically in the image. A central bulge is visible, exhibiting a smoother, more concentrated distribution of light. The disk component appears less uniform, showing subtle mottling that may indicate spiral arm structures, though these are not clearly defined. The overall color profile suggests a mix of stellar populations, with the bulge exhibiting a slightly redder hue relative to the bluer color observed in the disk. This color variation is suggestive of older stars being centrally concentrated, whereas the star formation is potentially occurring throughout the disk structure. There appears to be some distortion of the disk from perfect planarity, which may suggest a weak tidal interaction. The disk exhibits a soft edge, with no significant dust lanes visible in the color bands. Overall, the galaxy appears relatively undisturbed, with only minor distortions to its smooth structure.
