The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, with a high degree of roundness and little evidence of a disk-like structure or spiral arms. The galaxy exhibits a color gradient, appearing yellower and brighter towards its core, suggesting an older stellar population dominating the central regions. The outer regions show a slight fading in intensity, creating a diffuse halo around the main body. There are no obvious signs of recent major mergers or significant tidal disturbances in the immediate vicinity.
