The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central bulge that appears yellowish in color, possibly indicating an older stellar population. The galaxy appears to be largely devoid of prominent spiral arms or significant dust lanes. A slight extension of the light on either side of the center could suggest the presence of a faint, diffuse disk component, however, the smoothness of the light distribution argues against this galaxy being a spiral type. There is no visual evidence of ongoing major mergers or tidal disturbances in this image, though subtle minor disturbances may not be readily apparent at this resolution. The overall appearance suggests the galaxy is likely an elliptical galaxy at moderate redshift.
