The galaxy presents a smooth, centrally concentrated morphology, appearing largely featureless in this image. Its overall shape approximates an elliptical form, displaying a slight elongation. The color profile indicates a predominantly red population of stars, suggesting an older stellar population and limited ongoing star formation. The galaxy exhibits a relatively high surface brightness, particularly in its core, indicative of a dense stellar concentration. There is no visual evidence of spiral arms, dust lanes, or other distinct structural features typically associated with spiral galaxies. The overall appearance suggests a relatively evolved system.
