The galaxy presents a generally smooth, elliptical morphology. It displays a central, concentrated bulge, gradually fading into an extended halo. The color appears relatively uniform across the galaxy, with a slight reddish tint, suggesting an older stellar population with reduced ongoing star formation. There is no obvious spiral arm structure or significant dust lane features visible. The overall appearance suggests a galaxy that is evolving passively, having largely exhausted its supply of gas for new star formation. There is very slight evidence of tidal disturbance. The galaxy appears as a fairly typical elliptical galaxy, with a well-defined, smooth structure and redder overall color.
