The galaxy presents as a flattened, disk-like structure oriented at an oblique angle relative to our line of sight. Its overall color appears to be dominated by yellowish and reddish hues, suggestive of an older stellar population. The central bulge region displays a concentrated, brighter, and yellower light, possibly indicative of a higher density of evolved stars. Faint bluish tints in the outer regions might indicate areas of younger star formation, albeit not prominent. The smoothness of the light distribution implies a lack of significant spiral arm structures or major dust lanes. There are subtle disturbances visible suggesting a minor gravitational interaction with another object. 
