The galaxy appears as a moderately inclined, disk-shaped structure. Its major axis is significantly longer than its minor axis, implying a flattened morphology. The central bulge is relatively prominent and exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, a diffuse, bluish disk is observed. The bluer colors indicate the presence of younger, hotter stars and ongoing star formation. The disk appears somewhat smooth and flocculent, lacking prominent spiral arm structures. Overall, this galaxy can be described as a disk galaxy with a substantial bulge, intermediate inclination, and moderate star formation activity within its disk.
