The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology without any discernible spiral arms or prominent dust lanes. A central bulge appears concentrated and exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions of the galaxy fade gently into the background, displaying a bluer tinge, which may suggest the presence of younger stars. The overall appearance suggests a galaxy of intermediate redshift, with a dominant spheroidal component. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in this image.
