The galaxy presents as a disk galaxy seen at an oblique angle. Its structure is moderately smooth, with a central bulge that appears elongated. There is little to no apparent spiral structure visible in this image. The color profile indicates an intermediate population of stars, with a subtle shift towards redder hues in the central bulge, suggesting a higher concentration of older stars in the nucleus. The lack of distinct blue regions or bright knots indicates a relatively low rate of on-going star formation. Based on its overall morphology, this could potentially be classified as an early-type spiral or lenticular galaxy. There are no obvious signs of tidal disturbances or interaction with other galaxies. 
