The galaxy appears to be a disk galaxy, observed at a high inclination. The central bulge region is noticeably brighter and more concentrated, exhibiting a yellowish hue, suggesting an older stellar population. The disk component is less defined, showing a subtle blue tint, hinting at more recent star formation. The galaxy appears relatively smooth, with no distinct spiral arm structure or prominent dust lanes visible in this image. The overall shape is elongated and slightly cigar-shaped. There is no obvious evidence of a major merger, although subtle asymmetries might indicate a minor interaction or disturbance. The galaxy's dimensions appear moderate.
