The galaxy presents an elongated, disk-like morphology, viewed at an oblique angle, between edge-on and face-on. The central region exhibits a concentrated, brighter luminosity indicative of a significant stellar population or potentially an active galactic nucleus. Moving outward from the center, the disk shows a radial color gradient transitioning from yellow to a more bluish hue, possibly indicating younger stellar populations in the outer regions, where there may be a hint of spiral arm structure. The color distribution suggests ongoing star formation within the disk. No significant tidal features or indications of a major merger event are apparent, although the shape is slightly irregular. The galaxy exhibits a smooth overall texture with no distinct dust lanes visible within the optical wavelength range captured by the image.
