The galaxy presents as a concentrated, bright, and largely featureless elliptical or lenticular form. There is a luminous central bulge that diminishes in intensity outward, showing no distinct spiral arms or bar structures. The galaxy appears to be a relatively smooth, single object with no obvious signs of on-going major mergers, although some minor disturbance or interaction cannot be entirely ruled out. The shape appears to be somewhat elongated, but largely rounded in form. Its color suggests a mature stellar population with moderate to low levels of on-going star formation. Overall, the galaxy appears to be a fairly regular and evolved system.
