The galaxy presents a generally smooth, elliptical morphology. It appears mostly round, with only a slight elongation. The color gradient suggests a concentration of older stellar populations towards the center, indicated by the reddish hue, while the outer regions exhibit a bluer tint, potentially indicating ongoing, albeit relatively subdued, star formation. There is no clear evidence of spiral arm structure or a prominent disk. No significant merger events or tidal disturbances are visually apparent, though there appears to be a very faint distortion or possible tidal tail feature along one side of the galaxy. Overall, the galaxy appears to be relatively undisturbed, and its light profile follows a fairly smooth distribution.
