The galaxy exhibits a morphology suggestive of an ongoing or recent merger. The primary body of the galaxy appears largely smooth and elliptical, with a concentrated central bulge. Emanating from this central region are what appear to be faint tidal features or disturbed spiral arms. The color profile indicates a population dominated by older stars, as evidenced by the reddish hues in the central bulge. However, there are patches of bluer light interspersed, hinting at regions of more recent star formation within the system. The overall light distribution seems to suggest a system in transition, potentially evolving from a spiral-like structure towards a more spheroidal form as a result of the gravitational interactions. There is visible asymmetry in the outer regions of the galaxy, indicative of ongoing dynamical processes.
