The galaxy presents a somewhat elliptical morphology, appearing largely smooth and relatively featureless at this resolution. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. There is a gradual decrease in luminosity moving outwards from the core.

The overall color profile appears to be tending toward redder hues, indicating an older stellar population with reduced ongoing star formation. Marginal evidence of disk-like structures, though not clearly defined, can be seen. No signs of major mergers are apparent, though minor disturbances cannot be ruled out. Overall, the galaxy exhibits a relatively relaxed morphology characteristic of an evolved system.
