The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The core exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, more diffuse bluish light extends outward from the central region, suggesting the presence of a younger stellar population and ongoing, though subdued, star formation in the outer regions. There's a slight elongation to the galaxy's overall shape, but it is generally round. No distinct spiral arms or bar structures are discernible. There is no obvious evidence of any major mergers or tidal disturbances.
