The galaxy appears to be a spiral galaxy, seen at a slight angle. It exhibits a bright, concentrated central bulge that appears yellowish-white, suggesting an older stellar population dominates the core. The spiral arms are not well-defined, appearing somewhat flocculent. There is some indication of blueish regions within the arms, indicative of younger, hotter stars and ongoing star formation. The galaxy’s overall color gradient shifts from the yellowish core to bluer hues in the outer arms, as expected in spiral galaxies with active star formation in the disk. There is no evidence of a strong bar structure and no apparent signs of major tidal disturbances or ongoing merging activity. The galaxy's overall structure suggests a relatively evolved system undergoing moderate star formation within its spiral arms.
