The galaxy appears to be a relatively smooth, disk-like structure. Its overall morphology suggests an elliptical galaxy, though there is a slight elongation. The color distribution indicates a higher concentration of older stars towards the center, implied by the yellowish hue. The outer regions display hints of bluer colors, which may indicate a small population of younger, hotter stars and ongoing star formation. There is no obvious evidence of significant spiral arms or major disturbances, such as tidal tails or mergers, within the observed image. The overall impression is of a galaxy that is mostly quiescent in terms of star formation, but still with small presence of new stars.
