This galaxy exhibits a prominent, bright central bulge, suggesting a significant concentration of older stellar populations. The overall color profile indicates a mix of stellar ages, with the core appearing more yellow and orange than the outer regions. Fainter, bluer regions possibly indicating star formation. The spiral structure appears faint and not very tightly wound. The disk structure exhibits an orientation angled slightly towards the viewer, but it is not quite edge-on. I do not notice any significant tidal tails or distortions, suggesting that recent major merger events are unlikely. However, there are a few faint irregularities along the periphery of the disk that *could* be the result of a past minor interaction or merger. No strong bar feature is visible in the center of the galaxy. Overall, the galaxy appears to be a relatively undisturbed spiral galaxy with a moderate bulge.
