The galaxy presents an elliptical morphology, appearing as a diffuse, somewhat flattened spheroid. The light distribution suggests a concentration towards the central region, indicating a possible bulge. Evidence of a disk component is present in the image, with a slight elongation and structure extending from the core. There appear to be faint features suggesting mild disturbances and asymmetry, indicative of potential minor mergers or interactions. The galaxy exhibits a color gradient, with bluer hues concentrated toward the center, possibly indicating younger stellar populations, and redder hues towards the outer regions, which may be representative of older stars. The presence of some brighter, unresolved knots and structures is evident, potentially due to star-forming regions.
