The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated light distribution, with the luminosity gradually decreasing towards the outer regions. There is little evidence of significant spiral arm structure or prominent dust lanes. The galaxy is generally round in shape.

The galaxy has a yellowish-orange hue. This color suggests a stellar population dominated by older, redder stars, which is consistent with a relatively low star formation rate. The galaxy is of substantial mass. There is no clear evidence of ongoing major mergers or significant tidal disturbances in this image, though some minor disturbance cannot be ruled out.
