The galaxy appears to be an elliptical galaxy, showing a generally smooth and diffuse light distribution. Its overall shape seems to be somewhat spheroidal but tending toward an elongated form. There is a concentration of light toward the center, suggesting a defined galactic nucleus. Colors observed are primarily in the green/blue/yellow bands, but the galaxy appears to be composed of older stars with low star formation activity. There is evidence of some minor disturbance that suggests the galaxy is possibly undergoing a minor merger or tidal interaction with another galaxy, but it is generally in a relaxed state. The galaxy does not present any strong signs of spiral arm structure or prominent dust lanes.