The galaxy presents as an elliptical-type morphology, appearing largely smooth and without prominent spiral arms or a well-defined disk structure. It exhibits a relatively high degree of central concentration with the luminosity appearing more condensed towards the core. The galaxy's color profile suggests a population of older stars, indicated by its redder hue, which aligns with a lower rate of current star formation. There's little visual evidence of on-going mergers or major disturbances in its structure. The galaxy shows an overall rounded shape, with some deviation towards an intermediate elliptical form.
