The galaxy appears as a concentrated, elliptical structure. It exhibits a smooth, centrally concentrated morphology with a yellowish hue, suggesting an older stellar population. There is a slight asymmetry and potentially some minor disturbances within the galaxy's outer regions. The roundness of the galaxy is somewhere in between round and elliptical. There is no obvious spiral arm structure visible. The galaxy appears relatively isolated, with no clear signs of a major ongoing merger with another significant galaxy. Some faint features possibly indicative of minor tidal interactions may be present. The galaxy's color suggests a moderate amount of ongoing star formation.
