This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. It appears generally round in shape with a slight ellipticity. There are no obvious spiral arm structures or significant dust lanes visible. The color profile suggests a population of older stars, with the galaxy emitting strongly in the redder bands, and weaker emission in the bluer bands. There is no evidence of recent major merger events or significant tidal disturbances, although the possibility of minor interactions with other galaxies cannot be excluded. It is likely to be of considerable mass. Star formation rates are estimated to be low.