The galaxy presents as a concentrated central bulge. It appears to be a disk galaxy, based on its faint edges with spiral arms. The light distribution is fairly smooth, with a yellow hue around the central region that indicates an older stellar population. Faint disk features can be seen which imply the potential for ongoing or recent star formation, although it seems to be primarily composed of older stars. The overall shape is tending toward round, rather than elongated, suggesting a classification along the lines of a relatively early-type spiral galaxy. There might be a hint of a minor disturbance in the galaxy's structure, but no signs of major merger activity are visible.
