The galaxy presents a notable disk structure, viewed at an angle somewhat inclined from edge-on. Within the disk, spiral arms are visible, exhibiting a somewhat flocculent or patchy morphology. A prominent central bulge is apparent, exhibiting a smooth, concentrated appearance. A bar structure appears to traverse the bulge region.

The color distribution suggests a mix of stellar populations, with a generally yellowish hue in the bulge region suggestive of older stars, and bluer colors in the disk and spiral arms, indicating ongoing star formation. There may be dust lanes running through the spiral arms, which contributes to the colors of the disk. No signs of any major mergers were identified.
