The galaxy presents as a concentrated, centrally brightened structure. It appears largely featureless, exhibiting a smooth light distribution without prominent spiral arms or a distinct bulge. The morphology appears mostly round, lacking any significant elongation or asymmetry. There is some evidence of a slight disturbance or minor irregularity in the galaxy's outer regions, but no major mergers or tidal features are immediately apparent. The overall color is somewhat redder, which might suggest an older stellar population and suppressed star formation activity.
