The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, displaying a gradual decrease in intensity outwards from the core. The dominant color is yellowish, suggesting a relatively older stellar population with fewer ongoing star-forming regions. There may be a faint disk present. There is no obvious evidence of spiral arm structure or significant dust lanes. No tidal features or signs of a major merger event are apparent. The shape is quite round. The galaxy's overall appearance indicates that it is likely a large, relatively massive system with a low rate of star formation.
