This galaxy exhibits a generally smooth morphology, appearing largely elliptical or spheroidal. The light distribution suggests a high degree of central concentration, with a bright, relatively compact core that diffuses outward. There is very little evidence of spiral arm structure or significant dust lanes. The galaxy appears fairly round in shape, with only a slight elongation discernible. A faint blue hue is observed within the galaxy, which may indicate some ongoing star formation. There are no obvious signs of a major ongoing merger event, although some slight asymmetries in the outer regions could hint at past interactions or minor disturbances. Overall, the galaxy seems to be a relatively evolved system.
