The galaxy presents as a predominantly smooth, elliptical morphology with a high degree of roundness. The color profile indicates a dominant population of older stars, with a yellowish hue concentrated towards the central region. There is a faint, diffuse halo extending outwards from the core, gradually fading into the background sky. No distinct spiral arm structures, dust lanes, or signs of recent major merger activity are discernible. There might be very minor disturbances present but these are not easily identifiable. The galaxy appears relatively isolated and undisturbed. Overall, it gives the impression of a well-evolved, quiescent system.