This galaxy appears to be a relatively smooth, round system. There is a bright, concentrated central bulge region that dominates the overall structure. The core color appears yellowish, potentially indicative of an older stellar population. A fainter, bluish halo surrounds the bulge, which could suggest the presence of a younger, more metal-poor stellar population or ongoing, though limited, star formation. There is no distinct spiral arm structure or bar visible, and the galaxy shows no signs of major tidal disturbances or mergers, although some very subtle minor asymmetry could potentially be present. It would be interesting to observe if there is any gas content and to confirm the estimates of stellar mass.
