The galaxy presents as a relatively large spiral system, displaying a prominent disk structure. The spiral arms are well-defined, exhibiting a somewhat flocculent morphology. Evidence suggests substantial ongoing star formation within these arms, as indicated by their bluish hue. The central bulge appears small to moderately sized and exhibits a yellowish coloration, which could suggest an older stellar population. The galaxy's orientation is close to face-on relative to our line of sight. No significant bar feature is immediately apparent within the central regions. There's no apparent major disturbance to the overall structure, which rules out a recent major merger. However, the possibility of minor tidal interactions can't be ruled out. Overall, the system appears to be a mature spiral galaxy with active star formation within its disk.
