The galaxy appears to be an elliptical galaxy, displaying a generally smooth and centrally concentrated morphology. The color profile suggests an older stellar population with a dominant redder hue, particularly concentrated towards the core. There is a slight elongation of the galaxy along one axis, but overall, it maintains a fairly rounded shape. No distinct spiral arms or significant dust lanes are discernible. There is no evidence of any major ongoing merging events or significant tidal disturbances within this field of view.
