The galaxy presents as a largely featureless, smooth structure with a concentrated central bulge. It appears nearly circular in projection, exhibiting high degree of rotational symmetry. There is little evidence of spiral arms or a distinct disk component. The overall color profile indicates a dominant population of older stars. The redder light is concentrated towards the central region of the galaxy, suggesting an aging stellar population, with blue light surrounding the center of the object. There are no indications of on-going major merging events.
