This galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge region that appears yellowish-orange in color, suggestive of an older stellar population with fewer young, hot stars. Extending outward from the central bulge, the galaxy displays a more diffuse halo that is bluer in color, possibly indicating the presence of a more recent, albeit low level, of star formation activity. The shape of the galaxy is elongated, appearing somewhat cigar-shaped. No distinct spiral arms or bar structures are readily apparent. There is no obvious indication of any major mergers or tidal disturbances in this image. The galaxy's overall structure suggests that it is an evolved system which is nearing the end of its star formation lifecycle.
