The galaxy exhibits an overall elliptical morphology, appearing largely smooth and centrally concentrated. There is a noticeable color gradient, transitioning from a yellow-orange core to a bluer, less intense outer halo. The core region dominates the galaxy's light profile, suggesting a concentrated stellar population. No distinct spiral arms or bar features are discernible. There is a slight elongation in its shape, deviating from a perfectly circular profile but appears generally rounded. No apparent tidal features or signs of a major merger event are present. The galaxy appears to be relatively isolated, showing no obvious interaction with nearby companions within the field of view. The faint blue halo may imply low-level ongoing star formation or an older population of stars.
