The galaxy presents as a relatively smooth, elliptical morphology, appearing largely featureless at this resolution. Its shape is approximately round, showing no significant elongation. The color gradient indicates a higher concentration of older stellar populations, giving it a reddish-yellow hue. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy does not appear to be undergoing any major merging activity, although subtle signs of minor disturbances cannot be entirely ruled out. Overall, the galaxy's morphology suggests it is a well-established, relatively quiescent system.
