This galaxy appears to be a grand design spiral galaxy with a relatively small bulge and a well-defined disk. The spiral arms are tightly wound near the center, becoming more open and less defined as they extend outward. Several spiral arms appear to be present, possibly more than four. The arms exhibit a mottled texture, suggesting the presence of active star formation regions. The central bulge is not particularly dominant, appearing as a moderate concentration of light. There is no obvious bar structure visible. The overall appearance suggests a relatively isolated galaxy with no signs of significant interaction or merging, though a minor disturbance in the disk's symmetry may be present. The galaxy's color suggests a diverse stellar population, with a mix of older, redder stars and younger, bluer stars concentrated in the spiral arms.
