The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The light distribution suggests a dominant spheroidal component. There is no apparent spiral arm structure or prominent dust lanes. The object displays a mostly uniform color gradient, shifting from a brighter, bluer core to a slightly redder, fainter outer halo. The overall morphology appears relaxed, indicating it is unlikely to be undergoing a major merger event, though minor disturbances cannot be ruled out. The galaxy is moderately luminous and likely possesses a substantial stellar mass. Star formation appears present but not dominant, as the core is a vibrant blue, but not bright enough to indicate substantial ongoing star formation. The galaxy's apparent shape is slightly elongated.
