The galaxy presents an elliptical morphology, appearing largely smooth in structure with a centrally concentrated bright core. The overall shape is predominantly round, with only slight deviations from perfect circularity. There is a distinct lack of prominent spiral arms or a well-defined disk component. The galaxy's color profile suggests a population of older stars, appearing relatively redder compared to actively star-forming galaxies. No obvious signs of ongoing major merging events are apparent. There may be a very slight disturbance in the galaxy’s morphology. The light profile fades gradually from the core outwards with no sharp edges.
