This galaxy appears to be a relatively smooth, elliptical galaxy at a redshift of approximately 0.16, suggesting a considerable distance. The galaxy presents a concentrated central bulge that gradually diffuses outward into a less defined halo. The color profile indicates a population dominated by older stars, with a yellowish hue dominating the structure. There is little evidence of spiral arms or significant dust lanes. It exhibits signs of minor disturbances but it doesn't appear to be undergoing any major mergers or interactions with other galaxies. The galaxy has an approximate diameter of 6 kpc. Based on these characteristics, this galaxy is most likely a passive elliptical galaxy, and the star formation rate is consistent with low levels of ongoing star formation. 
