The galaxy exhibits an overall elliptical morphology, appearing largely smooth in structure. Its light profile suggests a concentration towards the center, with a gradual decrease in intensity towards the outer regions. The core appears intensely luminous, displaying a bright, almost stellar-like central component. Emanating outward from the core is diffuse, orange and yellow-shifted light that is likely older stellar populations. This light is somewhat disrupted, leading to distorted shape. The overall color suggests a evolved system dominated by intermediate to old stars. The is evidence of an on-going or past merging event or tidal disruption, altering the overall symmetry and creating some irregularities in the outer isophotes. This is supported by a faint bluish component that is potentially due to areas of recent star formation within the galaxy, though it could also be light from the core.
