The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. There is very little evidence of spiral arms or a disk. It appears to be quite luminous, with a color gradient suggesting an older stellar population dominating the light output, likely resulting in low star formation. The galaxy is relatively round in shape. There are no apparent major distortions or tidal tails indicative of an ongoing or recent major merger event, although the possibility of minor disturbances within the system cannot be entirely ruled out. The galaxy appears to be a fairly isolated system within its immediate vicinity.
