The galaxy presents as a largely smooth, elliptical structure. Its core appears bright and concentrated, exhibiting a yellowish hue that suggests an older stellar population. The isophotes are generally rounded, but with a slight ellipticity. There is a subtle color gradient visible, with the outer regions appearing somewhat bluer, possibly indicating the presence of a younger stellar population or ongoing low-level star formation. No prominent spiral arms or significant dust lanes are discernible. The overall morphology suggests this galaxy is a relatively massive system that is not currently undergoing major merging activity. Minor disturbances cannot be ruled out due to the image resolution.
