The galaxy presents a disk-like morphology, though the image resolution limits a definitive classification. There is evidence of a central bulge exhibiting a yellowish hue, suggesting an older stellar population. The disk component appears more bluish, indicative of ongoing star formation. While some structure is present, it does not appear as a grand design spiral. There's a slight asymmetry that could be due to a minor disturbance. There is no strong evidence of an ongoing major merger or tidal features. The galaxy presents a relatively smooth appearance, lacking significant dust lanes or prominent star-forming regions.
