The galaxy presents a generally smooth morphology, with a dominant central bulge. The galaxy appears elliptical, but not perfectly rounded, and there are no spiral arms readily visible. There is a noticeable color gradient from the center outwards; the central bulge is a more luminous yellow, indicative of an older stellar population, transitioning to a fainter, redder hue in the outer regions, which may indicate regions of dust obscuration or a population of less massive stars. The galaxy exhibits no signs of major ongoing mergers or significant tidal disturbances, however there may be some minor asymmetry in its shape, which could be the result of an old merger event. The galaxy has a red shift of z~0.27. Given the lack of obvious star formation indicators and generally smooth morphology, it is likely to be a relatively quiescent galaxy.