The galaxy appears to be an elliptical type, characterized by a relatively smooth and featureless light distribution. Its morphology is largely spheroidal, with some deviation from perfect roundness, tending towards an intermediate shape between circular and elongated. There appears to be little to no discernible disk component.

There are no obvious signs of spiral arms or significant dust lanes. Minor disturbances may be present within the galactic structure. There is no clear evidence of a major merger event or ongoing significant interaction with another galaxy. The stellar population appears somewhat evolved, indicated by the redder color index. The galaxy appears to be of significant mass, exhibiting a measurable, but not exceptionally high, rate of star formation.
