The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The light distribution is fairly uniform, lacking significant features such as spiral arms or distinct star-forming regions. The color appears moderately red, suggesting an older stellar population and relatively low current star formation. The overall shape is mostly round, with a slight deviation towards an elongated form. There is no obvious evidence of ongoing major mergers or significant tidal disturbances, although subtle irregularities may indicate minor interactions in the past.
