The galaxy presents as a centrally concentrated object with a smooth, featureless morphology. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color transitions to a faint bluish tinge, potentially indicative of a younger stellar population or a degree of ongoing star formation within the galactic disk. There are no apparent spiral arms or bar structures visible. The galaxy appears to be relatively isolated, with no obvious signs of major gravitational disturbance or ongoing merger activity, although subtle asymmetries in the outer regions might suggest minor interactions. Its overall shape appears more elliptical than disk-like, and it is moderately extended on the image. 
