The galaxy presents as an elliptical morphology, exhibiting a smooth and relatively featureless structure. Its light profile is centrally concentrated, with a gradual decline in luminosity towards its outer regions. The object displays a redder color, suggesting a stellar population dominated by older, evolved stars. There is a slight elongation observed in the galaxy's shape, but it generally appears fairly round. No apparent signs of ongoing major mergers or significant tidal disturbances are visible. There is very little evidence of spiral arms or a prominent disk component. The absence of strong blue light suggests a low rate of current star formation.
