This galaxy presents a centrally concentrated morphology, appearing largely smooth in overall structure. The core exhibits a bright, diffuse glow, suggesting a high stellar density or potentially an active galactic nucleus, though further spectroscopic data would be needed to confirm the latter. Moving outward from the center, the light distribution gradually diminishes. There is a hint of asymmetry in the outer regions of the galaxy, with a slightly elongated shape, which may suggest minor tidal interaction or internal dynamical processes. I do not see a disk structure. The overall color of the galaxy is yellowish, indicating a relatively old stellar population. Possible faint, minor disturbances exist on the edge of the galaxy, suggesting a merger history but this may be noise. Further imaging at greater resolution would be required to ascertain the nature of these disturbances.
