This galaxy appears to be a spiral type, exhibiting a moderately sized bulge and a prominent, relatively well-defined disk structure. I observe two apparent spiral arms. These arms have a moderately wound appearance and appear to emanate from the central bulge region. The color distribution suggests a mix of stellar populations. The bulge exhibits a yellowish hue, indicative of older, redder stars, whereas the spiral arms contain regions of bluish light, hinting at ongoing star formation. There may be a faint bar structure visible in the central region. I also note what may be a merger or tidal disruption.
