The galaxy presents as a relatively smooth, disk-like structure with a prominent central bulge. It is oriented with its major axis along the horizontal plane in the image. The bulge exhibits a yellow-red hue, suggesting a population of older stars. The disk appears bluer in color than the central bulge, consistent with the presence of younger, hotter stars and ongoing star formation.

The shape is generally elliptical, deviating slightly from a perfect circle. There is no obvious sign of a spiral arm structure or a bar. No significant tidal features or distortions are visible, indicating that the galaxy is likely not undergoing a major merger event. However, a subtle asymmetry exists, with a slight warp apparent.
