The galaxy presents a predominantly smooth morphology with a centrally concentrated light profile. It appears largely spheroidal, with a high degree of central symmetry. A faint blue halo is present, which may indicate some active star formation, but is more likely a result of image distortion. There is no clear evidence of spiral arms or a distinct disk structure within the limits of the image resolution. There is no indication of any major disturbance or tidal features to suggest a recent major merger event. The galaxy appears relatively isolated, without any visually interacting galaxies in close proximity. The overall color suggests a relatively evolved stellar population, but the faint blue halo suggests that the galaxy has not completely quenched star formation.