The galaxy appears to be a spiral galaxy, viewed at an intermediate angle. There are faint spiral arms visible in the outer disk region. The central bulge is prominent and exhibits a smooth, concentrated light distribution, with a bright yellow/white hue indicating a high density of older stars. The disk shows a bluer color, potentially indicating some on-going star formation within the spiral arms. Overall, the galaxy has a slightly elliptical shape. No major signs of active galactic nuclei or tidal disturbances are visually apparent in the image. The red shift value suggests the galaxy is relatively close to us.