The galaxy appears to be an elliptical galaxy, characterized by a smooth, symmetrical structure. It exhibits a concentrated central bulge, with the light intensity decreasing gradually towards the outer regions. The overall color is yellowish, suggesting an older stellar population with lower levels of ongoing star formation. There are no prominent spiral arms or distinct dust lanes visible. The galaxy appears relatively isolated, with no clear signs of major tidal interactions or ongoing mergers. The isophotes are generally round, indicating a minimal degree of ellipticity. There may be a faint, extended halo surrounding the main body of the galaxy, but the signal is weak and requires further analysis to confirm. The lack of observable features suggests a quiescent galaxy with a high degree of dynamical stability.
