The galaxy presents a disk-like morphology with a relatively bright central bulge region that appears yellowish in color. This suggests a concentration of older stars in the galactic center. Two loosely defined spiral arms extend from the bulge, showing hints of blueish regions, implying the presence of younger, hotter stars and star-forming regions within those arms. The disk exhibits a noticeable tilt relative to the observer's line of sight. The overall shape appears somewhat elliptical, with a major to minor axis ratio less than one. The winding of the spiral arms seems medium to tight, and the disk shows no major signs of recent disturbance or merging activity, though a minor asymmetry may be present. Dust lanes are not prominently visible, though some mottled texture is observed in the disk.
