The galaxy presents as a centrally concentrated object, likely an elliptical, with a smooth, diffuse halo. The core region exhibits a yellowish-orange hue, suggesting an older stellar population and a low rate of star formation, if any. The outer regions of the galaxy have a blueish tinge, possibly indicating the presence of younger stars, or a recent, minor merger event that has introduced new gas for star formation, albeit not dramatically influencing the overall galactic morphology. There are no clear signs of spiral arms, bar structures, or prominent dust lanes; however, there is a slight elongation in the shape, indicating it is not perfectly spherical. It is possible that some minor gravitational interaction could be occurring. There do not appear to be any significant tidal tails or indications of major disturbances. The galaxy is relatively isolated in the field, which suggests a high likelihood that the object is not in a stage of major merging or interaction. 
