The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The light distribution appears elongated, with a cigar-shaped profile, suggesting it might be a prolate spheroid. A slight color gradient is observed with a central region exhibiting a yellowish hue and the outer regions appear more blueish. There are no obvious signs of strong spiral arm structures, bars, or a prominent central dust lane. The galaxy appears relatively undisturbed, with no clear indications of ongoing major mergers or tidal interactions. Some minor disturbances cannot be ruled out.
