The galaxy presents as a single, largely homogenous, elliptical-like object with a smooth appearance. It is highly concentrated, with a bright central core that gradually diffuses outwards. There is a slight color gradient, with the core exhibiting a more yellow hue and the outer regions trending towards a redder color. There is no readily apparent spiral arm structure or significant dust lane obscuration, suggesting the light is emitted predominately by an older stellar population with a low star formation rate. The overall morphology suggests this galaxy is a relaxed system, with no visible tidal features indicative of recent major merger activity. There appears to be a slight, but non-obvious redder halo surrounding it.
