The galaxy presents as an elliptical morphology with a smooth light distribution, concentrated toward the center. The main body of the galaxy exhibits a yellow-white hue, with no clear indications of spiral arms or a defined disk structure. There is evidence of a potential disturbance or feature at one end of the galaxy, appearing as a redder, less defined region possibly indicating an area of increased star formation or interaction. The overall color suggests a population of older stars, with a moderate amount of ongoing star formation. The galaxy is primarily smooth with a somewhat round morphology. There is no distinct evidence of a major ongoing merger.
