The galaxy presents a predominantly elliptical morphology, displaying a smooth, centrally concentrated light profile with minimal discernible substructure. The galaxy's color appears relatively red, suggesting an older stellar population and a low rate of ongoing star formation. The shape deviates slightly from a perfect circle, showing a moderate ellipticity. A faint, diffuse halo may extend beyond the main body of the galaxy, though the image resolution limits precise characterization. The overall appearance points towards a galaxy that has largely completed its major merging activity and is evolving passively.
