The galaxy presents as a disk-shaped structure, viewed at an oblique angle. A prominent central bulge is observed, exhibiting a higher concentration of light than the surrounding disk. The disk component reveals a discernible spiral arm structure, although somewhat diffuse and not sharply defined. The overall color of the galaxy appears to be skewed towards the redder end of the spectrum, suggesting a relatively older stellar population. There appears to be a dust lane running along the major axis of the galaxy, partially obscuring the light from the bulge and inner disk. The galaxy exhibits a low ellipticity, suggesting that it is closer to being face-on than edge-on. There is no evidence of active star formation in the image.
