The galaxy presents as a centrally concentrated elliptical system, exhibiting a smooth, featureless morphology with a notable lack of spiral arms or distinct substructure. The galaxy's color profile suggests a population dominated by older stars, with a redder hue in the core gradually fading toward the outer regions. The galaxy's shape appears roughly rounded with a hint of ellipticity. There are no prominent signs of ongoing major mergers or significant tidal disturbances in its immediate vicinity, suggesting it is a relatively isolated and relaxed system.
