The galaxy presents a generally smooth and rounded morphology. It appears to be an elliptical galaxy, though a subtle disk component may be present. There is little evidence of significant star formation activity within the central region, indicated by a primarily yellowish hue. The central bulge is prominent and concentrated, gradually fading into the outer regions of the galaxy. Some of the more redshifted, less luminous light is seen in the halo around the galaxy, and the slight asymmetry may indicate a small merging event has recently occurred. 
