The galaxy presents a generally smooth, elliptical morphology. There is a central concentration of light, appearing yellowish-orange in color, which likely indicates an older stellar population. The outer regions of the galaxy exhibit a gradual decrease in surface brightness and a slight shift toward a greenish hue, suggesting the presence of some younger stars or potentially ongoing star formation. No distinct spiral arms or bar structures are discernible. The overall shape is mostly round, showing only a very slight elongation. There is no visually apparent evidence of major mergers or tidal disturbances, although subtle irregularities in the outer halo cannot be entirely ruled out given the image resolution.
