The galaxy presents as a roughly elliptical structure, with a significant central bulge. It is characterized by a smooth, diffuse light profile, indicative of an older stellar population. There's a subtle elongation, suggesting it could be classified as an elliptical galaxy that is not perfectly spherical. The core exhibits a higher concentration of light, and a slightly yellowish hue compared to its surrounding regions. The outer edges of the galaxy fade gently into the background sky, and there is little evidence of spiral arm structures or ongoing star formation in this image, which aligns with the yellowish color associated with older stars. There is a hint of asymmetry in its overall form, suggesting possible minor gravitational interactions or tidal disturbances.
