The galaxy appears as a somewhat elongated, disk-shaped structure oriented approximately vertically in the image. A prominent central bulge exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. The disk is visible, displaying a bluish hue, possibly indicating the presence of younger, hotter stars and ongoing star formation. While there is some evidence of a disk, it doesn't appear to have well-defined spiral arms. The structure seems somewhat disturbed, possibly exhibiting minor tidal features or asymmetries that could suggest past interactions or minor mergers. There is no clear evidence of a major ongoing merger, but the shape deviates somewhat from a perfectly smooth disk. Overall, the galaxy's appearance points towards a disk galaxy with a significant bulge, showing some signs of recent star formation.
