The galaxy appears to be an elliptical galaxy exhibiting a smooth, centrally concentrated light profile. Its overall shape is moderately elliptical, trending away from a perfect circle. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy displays a fairly uniform color, suggesting an older stellar population with minimal ongoing star formation. There might be very slight color variations that suggest subtle differences in stellar populations within the galaxy, but high resolution imagery would be required to confirm that. There is no obvious evidence of a major merger, although a minor tidal interaction or previous minor merger cannot be completely ruled out based on this image alone.
