The galaxy presents a generally smooth morphology with a centrally concentrated luminosity profile. The shape is more in-between rounded and elongated than a perfectly circular distribution. There is no strong evidence of spiral arms or other distinct features within the galaxy, suggesting it is likely an elliptical galaxy or a lenticular galaxy viewed at a high inclination. The galaxy exhibits a color gradient, appearing bluer in the central regions and slightly redder towards the outer edges. The absence of significant disturbances in the galaxy's structure indicates it is likely not undergoing a major merger event. Faint asymmetries might be present in the outer isophotes, suggesting possible minor interactions or past merger events.
