The galaxy presents as a centrally concentrated, smooth structure, strongly suggestive of an elliptical morphology. There is a clear radial color gradient, with the core exhibiting a yellowish hue which transitions to a slightly bluer color in the outer regions. This could indicate a change in stellar population with age and metallicity, with the core potentially containing older, metal-rich stars. The shape appears mostly round, with a slight suggestion of elongation. There are no obvious signs of spiral arms or dust lanes within the galaxy. There is a small amount of low surface brightness extensions of the galaxy. No strong tidal features or signs of a major merger are apparent within the immediate vicinity of the galaxy, though minor disturbances cannot be ruled out. At its estimated distance, this galaxy would be a large and fairly massive system.
