The observed galaxy exhibits an approximate elliptical morphology, with a bright, concentrated core. The central region shows a strong emission signature, likely indicating a high density of stars and/or the presence of an active galactic nucleus. Moving outwards from the core, the light profile appears to diminish gradually. The structure reveals subtle features suggestive of a possible minor disturbance or interaction event. The shape of the galaxy is somewhat asymmetrical; I note a possible warp in the galactic disk on the left. Evidence of a merger is present in the form of a bridge like appendage.
