The galaxy presents an elliptical morphology, with a smooth light distribution. The object is centrally concentrated, displaying a bright, yellowish core which indicates a high concentration of older stellar populations. The galaxy exhibits a gradual decrease in luminosity outwards from the core, with a faint halo extending beyond the central region. There is an indication of slight elongation of the galaxy's structure, suggestive of a somewhat cigar-like shape, but the overall morphology is still fairly spheroidal. There are no obvious signs of spiral arms or strong dust lanes. No evidence of major merger activity is apparent. Subtle irregularities in the outer regions may suggest minor disturbances.
